SOPHI

PHI HRT Data Table

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(Please check SOPHI page / contact SOPHI Support for detailed information)

DID Date Notes Description
243030101
20220303T094009
ISS off Degraded spatial resolution & polarimetric sensitivity
243030102
20220303T094309
ISS off Degraded spatial resolution & polarimetric sensitivity
243030103
20220303T094609
ISS off Degraded spatial resolution & polarimetric sensitivity
243030104
20220303T094909
ISS off Degraded spatial resolution & polarimetric sensitivity
243030105
20220303T095209
ISS off Degraded spatial resolution & polarimetric sensitivity
243030106
20220303T095509
ISS off Degraded spatial resolution & polarimetric sensitivity
243030107
20220303T095809
ISS off Degraded spatial resolution & polarimetric sensitivity
243030108
20220303T100109
ISS off Degraded spatial resolution & polarimetric sensitivity
243030109
20220303T100409
ISS off Degraded spatial resolution & polarimetric sensitivity
243030110
20220303T100709
ISS off Degraded spatial resolution & polarimetric sensitivity
243030111
20220303T101009
ISS off Degraded spatial resolution & polarimetric sensitivity
243030112
20220303T101309
ISS off Degraded spatial resolution & polarimetric sensitivity
243030113
20220303T101609
ISS off Degraded spatial resolution & polarimetric sensitivity
243030114
20220303T101909
ISS off Degraded spatial resolution & polarimetric sensitivity
243030115
20220303T102209
ISS off Degraded spatial resolution & polarimetric sensitivity
243030116
20220303T102509
ISS off Degraded spatial resolution & polarimetric sensitivity
243040101
20220304T104509
ISS off Degraded spatial resolution & polarimetric sensitivity
243040102
20220304T104810
ISS off Degraded spatial resolution & polarimetric sensitivity
243040103
20220304T105110
ISS off Degraded spatial resolution & polarimetric sensitivity
243040104
20220304T105410
ISS off Degraded spatial resolution & polarimetric sensitivity
243040105
20220304T105710
ISS off Degraded spatial resolution & polarimetric sensitivity
243040106
20220304T110010
ISS off Degraded spatial resolution & polarimetric sensitivity
243040107
20220304T110310
ISS off Degraded spatial resolution & polarimetric sensitivity
243040108
20220304T110609
ISS off Degraded spatial resolution & polarimetric sensitivity
243040109
20220304T110909
ISS off Degraded spatial resolution & polarimetric sensitivity
243040110
20220304T111209
ISS off Degraded spatial resolution & polarimetric sensitivity
243040111
20220304T111509
ISS off Degraded spatial resolution & polarimetric sensitivity
243040112
20220304T111809
ISS off Degraded spatial resolution & polarimetric sensitivity
243040113
20220304T112109
ISS off Degraded spatial resolution & polarimetric sensitivity
243040114
20220304T112409
ISS off Degraded spatial resolution & polarimetric sensitivity
243040115
20220304T112709
ISS off Degraded spatial resolution & polarimetric sensitivity
243040116
20220304T113009
ISS off Degraded spatial resolution & polarimetric sensitivity
243040117
20220304T113309
ISS off Degraded spatial resolution & polarimetric sensitivity
243040118
20220304T113609
ISS off Degraded spatial resolution & polarimetric sensitivity
243040119
20220304T113909
ISS off Degraded spatial resolution & polarimetric sensitivity
243050101
20220305T152009
ISS off Degraded spatial resolution & polarimetric sensitivity
243050102
20220305T152309
ISS off Degraded spatial resolution & polarimetric sensitivity
243050103
20220305T152609
ISS off Degraded spatial resolution & polarimetric sensitivity
243050104
20220305T152909
ISS off Degraded spatial resolution & polarimetric sensitivity
243050105
20220305T153209
ISS off Degraded spatial resolution & polarimetric sensitivity
243050106
20220305T153509
ISS off Degraded spatial resolution & polarimetric sensitivity
243050107
20220305T153809
ISS off Degraded spatial resolution & polarimetric sensitivity
243050108
20220305T154109
ISS off Degraded spatial resolution & polarimetric sensitivity
243050109
20220305T154409
ISS off Degraded spatial resolution & polarimetric sensitivity
243050110
20220305T154709
ISS off Degraded spatial resolution & polarimetric sensitivity
243050111
20220305T155009
ISS off Degraded spatial resolution & polarimetric sensitivity
243050112
20220305T155309
ISS off Degraded spatial resolution & polarimetric sensitivity
243050113
20220305T155609
ISS off Degraded spatial resolution & polarimetric sensitivity
243050114
20220305T155909
ISS off Degraded spatial resolution & polarimetric sensitivity
243050115
20220305T160209
ISS off Degraded spatial resolution & polarimetric sensitivity
243050116
20220305T160509
ISS off Degraded spatial resolution & polarimetric sensitivity
243050117
20220305T160809
ISS off Degraded spatial resolution & polarimetric sensitivity
243050118
20220305T161109
ISS off Degraded spatial resolution & polarimetric sensitivity
243050119
20220305T161409
ISS off Degraded spatial resolution & polarimetric sensitivity
243050120
20220305T161709
ISS off Degraded spatial resolution & polarimetric sensitivity
243060101
20220306T170509
ISS off Degraded spatial resolution & polarimetric sensitivity
243060102
20220306T170609
ISS off Degraded spatial resolution & polarimetric sensitivity
243060103
20220306T170709
ISS off Degraded spatial resolution & polarimetric sensitivity
243060104
20220306T170809
ISS off Degraded spatial resolution & polarimetric sensitivity
243060105
20220306T170909
ISS off Degraded spatial resolution & polarimetric sensitivity
243060106
20220306T171009
ISS off Degraded spatial resolution & polarimetric sensitivity
243060107
20220306T171109
ISS off Degraded spatial resolution & polarimetric sensitivity
243060108
20220306T171209
ISS off Degraded spatial resolution & polarimetric sensitivity
243060109
20220306T171309
ISS off Degraded spatial resolution & polarimetric sensitivity
243060110
20220306T171409
ISS off Degraded spatial resolution & polarimetric sensitivity
243060111
20220306T171509
ISS off Degraded spatial resolution & polarimetric sensitivity
243060112
20220306T171609
ISS off Degraded spatial resolution & polarimetric sensitivity
243060113
20220306T171709
ISS off Degraded spatial resolution & polarimetric sensitivity
243060114
20220306T171809
ISS off Degraded spatial resolution & polarimetric sensitivity
243060115
20220306T171909
ISS off Degraded spatial resolution & polarimetric sensitivity
243060116
20220306T172009
ISS off Degraded spatial resolution & polarimetric sensitivity
243060117
20220306T172109
ISS off Degraded spatial resolution & polarimetric sensitivity
243060118
20220306T172209
ISS off Degraded spatial resolution & polarimetric sensitivity
243060119
20220306T172309
ISS off Degraded spatial resolution & polarimetric sensitivity
243060120
20220306T172409
ISS off Degraded spatial resolution & polarimetric sensitivity
243060121
20220306T172509
ISS off Degraded spatial resolution & polarimetric sensitivity
243060122
20220306T172609
ISS off Degraded spatial resolution & polarimetric sensitivity
243060123
20220306T172709
ISS off Degraded spatial resolution & polarimetric sensitivity
243060124
20220306T172809
ISS off Degraded spatial resolution & polarimetric sensitivity
243060125
20220306T172909
ISS off Degraded spatial resolution & polarimetric sensitivity
243060126
20220306T173009
ISS off Degraded spatial resolution & polarimetric sensitivity
243060127
20220306T173109
ISS off Degraded spatial resolution & polarimetric sensitivity
243060128
20220306T173209
ISS off Degraded spatial resolution & polarimetric sensitivity
243060129
20220306T173309
ISS off Degraded spatial resolution & polarimetric sensitivity
243060130
20220306T173409
ISS off Degraded spatial resolution & polarimetric sensitivity
243060131
20220306T173509
ISS off Degraded spatial resolution & polarimetric sensitivity
243060132
20220306T173609
ISS off Degraded spatial resolution & polarimetric sensitivity
243060133
20220306T173709
ISS off Degraded spatial resolution & polarimetric sensitivity
243060134
20220306T173809
ISS off Degraded spatial resolution & polarimetric sensitivity
243060135
20220306T173909
ISS off Degraded spatial resolution & polarimetric sensitivity
243060136
20220306T174009
ISS off Degraded spatial resolution & polarimetric sensitivity
243060137
20220306T174109
ISS off Degraded spatial resolution & polarimetric sensitivity
243060138
20220306T174209
ISS off Degraded spatial resolution & polarimetric sensitivity
243060139
20220306T174309
ISS off Degraded spatial resolution & polarimetric sensitivity
243060140
20220306T174409
ISS off Degraded spatial resolution & polarimetric sensitivity
243060141
20220306T174509
ISS off Degraded spatial resolution & polarimetric sensitivity
243060142
20220306T174609
ISS off Degraded spatial resolution & polarimetric sensitivity
243060143
20220306T174709
ISS off Degraded spatial resolution & polarimetric sensitivity
243060144
20220306T174809
ISS off Degraded spatial resolution & polarimetric sensitivity
243060145
20220306T174909
ISS off Degraded spatial resolution & polarimetric sensitivity
243060146
20220306T175009
ISS off Degraded spatial resolution & polarimetric sensitivity
243060147
20220306T175109
ISS off Degraded spatial resolution & polarimetric sensitivity
243060148
20220306T175209
ISS off Degraded spatial resolution & polarimetric sensitivity
243060149
20220306T175309
ISS off Degraded spatial resolution & polarimetric sensitivity
243060150
20220306T175409
ISS off Degraded spatial resolution & polarimetric sensitivity
243060151
20220306T175509
ISS off Degraded spatial resolution & polarimetric sensitivity
243060152
20220306T175609
ISS off Degraded spatial resolution & polarimetric sensitivity
243060153
20220306T175709
ISS off Degraded spatial resolution & polarimetric sensitivity
243060154
20220306T175809
ISS off Degraded spatial resolution & polarimetric sensitivity
243060155
20220306T175909
ISS off Degraded spatial resolution & polarimetric sensitivity
243060156
20220306T180009
ISS off Degraded spatial resolution & polarimetric sensitivity
243060157
20220306T180109
ISS off Degraded spatial resolution & polarimetric sensitivity
243060158
20220306T180209
ISS off Degraded spatial resolution & polarimetric sensitivity
243060159
20220306T180309
ISS off Degraded spatial resolution & polarimetric sensitivity
243060160
20220306T180409
ISS off Degraded spatial resolution & polarimetric sensitivity
243070101
20220307T000009
ISS off Degraded spatial resolution & polarimetric sensitivity
243070102
20220307T000109
ISS off Degraded spatial resolution & polarimetric sensitivity
243070103
20220307T000209
ISS off Degraded spatial resolution & polarimetric sensitivity
243070104
20220307T000309
ISS off Degraded spatial resolution & polarimetric sensitivity
243070105
20220307T000409
ISS off Degraded spatial resolution & polarimetric sensitivity
243070106
20220307T000509
ISS off Degraded spatial resolution & polarimetric sensitivity
243070107
20220307T000609
ISS off Degraded spatial resolution & polarimetric sensitivity
243070108
20220307T000709
ISS off Degraded spatial resolution & polarimetric sensitivity
243070109
20220307T000809
ISS off Degraded spatial resolution & polarimetric sensitivity
243070110
20220307T000909
ISS off Degraded spatial resolution & polarimetric sensitivity
243070111
20220307T001009
ISS off Degraded spatial resolution & polarimetric sensitivity
243070112
20220307T001109
ISS off Degraded spatial resolution & polarimetric sensitivity
243070113
20220307T001209
ISS off Degraded spatial resolution & polarimetric sensitivity
243070114
20220307T001309
ISS off Degraded spatial resolution & polarimetric sensitivity
243070115
20220307T001409
ISS off Degraded spatial resolution & polarimetric sensitivity
243070116
20220307T001509
ISS off Degraded spatial resolution & polarimetric sensitivity
243070117
20220307T001609
ISS off Degraded spatial resolution & polarimetric sensitivity
243070118
20220307T001709
ISS off Degraded spatial resolution & polarimetric sensitivity
243070119
20220307T001809
ISS off Degraded spatial resolution & polarimetric sensitivity
243070120
20220307T001909
ISS off Degraded spatial resolution & polarimetric sensitivity
243070121
20220307T002009
ISS off Degraded spatial resolution & polarimetric sensitivity
243070122
20220307T002109
ISS off Degraded spatial resolution & polarimetric sensitivity
243070123
20220307T002209
ISS off Degraded spatial resolution & polarimetric sensitivity
243070124
20220307T002309
ISS off Degraded spatial resolution & polarimetric sensitivity
243070125
20220307T002409
ISS off Degraded spatial resolution & polarimetric sensitivity
243070126
20220307T002509
ISS off Degraded spatial resolution & polarimetric sensitivity
243070127
20220307T002609
ISS off Degraded spatial resolution & polarimetric sensitivity
243070128
20220307T002709
ISS off Degraded spatial resolution & polarimetric sensitivity
243070129
20220307T002809
ISS off Degraded spatial resolution & polarimetric sensitivity
243070130
20220307T002909
ISS off Degraded spatial resolution & polarimetric sensitivity
243070131
20220307T003009
ISS off Degraded spatial resolution & polarimetric sensitivity
243070132
20220307T003109
ISS off Degraded spatial resolution & polarimetric sensitivity
243070133
20220307T003209
ISS off Degraded spatial resolution & polarimetric sensitivity
243070134
20220307T003309
ISS off Degraded spatial resolution & polarimetric sensitivity
243070135
20220307T003409
ISS off Degraded spatial resolution & polarimetric sensitivity
243070136
20220307T003509
ISS off Degraded spatial resolution & polarimetric sensitivity
243070137
20220307T003609
ISS off Degraded spatial resolution & polarimetric sensitivity
243070138
20220307T003709
ISS off Degraded spatial resolution & polarimetric sensitivity
243070139
20220307T003809
ISS off Degraded spatial resolution & polarimetric sensitivity
243070140
20220307T003909
ISS off Degraded spatial resolution & polarimetric sensitivity
243070141
20220307T004009
ISS off Degraded spatial resolution & polarimetric sensitivity
243070142
20220307T004109
ISS off Degraded spatial resolution & polarimetric sensitivity
243070143
20220307T004209
ISS off Degraded spatial resolution & polarimetric sensitivity
243070144
20220307T004309
ISS off Degraded spatial resolution & polarimetric sensitivity
243070145
20220307T004409
ISS off Degraded spatial resolution & polarimetric sensitivity
243070156
20220307T005509
ISS off Degraded spatial resolution & polarimetric sensitivity
243070158
20220307T005709
ISS off Degraded spatial resolution & polarimetric sensitivity
243070159
20220307T005809
ISS off Degraded spatial resolution & polarimetric sensitivity
243070160
20220307T005909
ISS off Degraded spatial resolution & polarimetric sensitivity
243070161
20220307T010009
ISS off Degraded spatial resolution & polarimetric sensitivity
243070162
20220307T010110
ISS off Degraded spatial resolution & polarimetric sensitivity
243070163
20220307T010209
ISS off Degraded spatial resolution & polarimetric sensitivity
243070164
20220307T010309
ISS off Degraded spatial resolution & polarimetric sensitivity
243070165
20220307T010409
ISS off Degraded spatial resolution & polarimetric sensitivity
243070166
20220307T010509
ISS off Degraded spatial resolution & polarimetric sensitivity
243070167
20220307T010609
ISS off Degraded spatial resolution & polarimetric sensitivity
243080601
20220308T000009
ISS off Degraded spatial resolution & polarimetric sensitivity
243080602
20220308T000109
ISS off Degraded spatial resolution & polarimetric sensitivity
243080603
20220308T000209
ISS off Degraded spatial resolution & polarimetric sensitivity
243080604
20220308T000309
ISS off Degraded spatial resolution & polarimetric sensitivity
243080605
20220308T000410
ISS off Degraded spatial resolution & polarimetric sensitivity
243080606
20220308T000509
ISS off Degraded spatial resolution & polarimetric sensitivity
243080607
20220308T000609
ISS off Degraded spatial resolution & polarimetric sensitivity
243080608
20220308T000709
ISS off Degraded spatial resolution & polarimetric sensitivity
243080609
20220308T000809
ISS off Degraded spatial resolution & polarimetric sensitivity
243080610
20220308T000909
ISS off Degraded spatial resolution & polarimetric sensitivity
243080611
20220308T001009
ISS off Degraded spatial resolution & polarimetric sensitivity
243080612
20220308T001109
ISS off Degraded spatial resolution & polarimetric sensitivity
243080613
20220308T001209
ISS off Degraded spatial resolution & polarimetric sensitivity
243080614
20220308T001309
ISS off Degraded spatial resolution & polarimetric sensitivity
243080615
20220308T001409
ISS off Degraded spatial resolution & polarimetric sensitivity
243080616
20220308T001509
ISS off Degraded spatial resolution & polarimetric sensitivity
243080617
20220308T001609
ISS off Degraded spatial resolution & polarimetric sensitivity
243080618
20220308T001709
ISS off Degraded spatial resolution & polarimetric sensitivity
243080619
20220308T001809
ISS off Degraded spatial resolution & polarimetric sensitivity
243080620
20220308T001909
ISS off Degraded spatial resolution & polarimetric sensitivity
243080621
20220308T002009
ISS off Degraded spatial resolution & polarimetric sensitivity
243080622
20220308T002109
ISS off Degraded spatial resolution & polarimetric sensitivity
243080623
20220308T002209
ISS off Degraded spatial resolution & polarimetric sensitivity
243080624
20220308T002309
ISS off Degraded spatial resolution & polarimetric sensitivity
243080625
20220308T002409
ISS off Degraded spatial resolution & polarimetric sensitivity
243080626
20220308T002509
ISS off Degraded spatial resolution & polarimetric sensitivity
243080627
20220308T002609
ISS off Degraded spatial resolution & polarimetric sensitivity
243080628
20220308T002709
ISS off Degraded spatial resolution & polarimetric sensitivity
243080629
20220308T002809
ISS off Degraded spatial resolution & polarimetric sensitivity
243080630
20220308T002909
ISS off Degraded spatial resolution & polarimetric sensitivity
243080631
20220308T003009
ISS off Degraded spatial resolution & polarimetric sensitivity
243080632
20220308T003109
ISS off Degraded spatial resolution & polarimetric sensitivity
243080633
20220308T003209
ISS off Degraded spatial resolution & polarimetric sensitivity
243080634
20220308T003309
ISS off Degraded spatial resolution & polarimetric sensitivity
243080635
20220308T003409
ISS off Degraded spatial resolution & polarimetric sensitivity
243080636
20220308T003509
ISS off Degraded spatial resolution & polarimetric sensitivity
243080637
20220308T003609
ISS off Degraded spatial resolution & polarimetric sensitivity
243080638
20220308T003709
ISS off Degraded spatial resolution & polarimetric sensitivity
243080639
20220308T003809
ISS off Degraded spatial resolution & polarimetric sensitivity
243080640
20220308T003909
ISS off Degraded spatial resolution & polarimetric sensitivity
243080641
20220308T004009
ISS off Degraded spatial resolution & polarimetric sensitivity
243080642
20220308T004109
ISS off Degraded spatial resolution & polarimetric sensitivity
243080643
20220308T004209
ISS off Degraded spatial resolution & polarimetric sensitivity
243080644
20220308T004309
ISS off Degraded spatial resolution & polarimetric sensitivity
243080645
20220308T004409
ISS off Degraded spatial resolution & polarimetric sensitivity
243080646
20220308T004509
ISS off Degraded spatial resolution & polarimetric sensitivity
243080647
20220308T004609
ISS off Degraded spatial resolution & polarimetric sensitivity
243080648
20220308T004709
ISS off Degraded spatial resolution & polarimetric sensitivity
243080649
20220308T004809
ISS off Degraded spatial resolution & polarimetric sensitivity
243080650
20220308T004909
ISS off Degraded spatial resolution & polarimetric sensitivity
243080651
20220308T005009
ISS off Degraded spatial resolution & polarimetric sensitivity
243080652
20220308T005109
ISS off Degraded spatial resolution & polarimetric sensitivity
243080653
20220308T005209
ISS off Degraded spatial resolution & polarimetric sensitivity
243080654
20220308T005309
ISS off Degraded spatial resolution & polarimetric sensitivity
243080655
20220308T005409
ISS off Degraded spatial resolution & polarimetric sensitivity
243080656
20220308T005509
ISS off Degraded spatial resolution & polarimetric sensitivity
243080657
20220308T005609
ISS off Degraded spatial resolution & polarimetric sensitivity
243080658
20220308T005709
ISS off Degraded spatial resolution & polarimetric sensitivity
243080659
20220308T005809
ISS off Degraded spatial resolution & polarimetric sensitivity
243080660
20220308T005909
ISS off Degraded spatial resolution & polarimetric sensitivity
243080661
20220308T010009
ISS off Degraded spatial resolution & polarimetric sensitivity
243080662
20220308T010109
ISS off Degraded spatial resolution & polarimetric sensitivity
243080663
20220308T010209
ISS off Degraded spatial resolution & polarimetric sensitivity
243080664
20220308T010309
ISS off Degraded spatial resolution & polarimetric sensitivity
243080665
20220308T010409
ISS off Degraded spatial resolution & polarimetric sensitivity
243080666
20220308T010509
ISS off Degraded spatial resolution & polarimetric sensitivity
243080667
20220308T010609
ISS off Degraded spatial resolution & polarimetric sensitivity
243080668
20220308T010709
ISS off Degraded spatial resolution & polarimetric sensitivity
243080669
20220308T010809
ISS off Degraded spatial resolution & polarimetric sensitivity
243080670
20220308T010909
ISS off Degraded spatial resolution & polarimetric sensitivity
243080671
20220308T011009
ISS off Degraded spatial resolution & polarimetric sensitivity
243080672
20220308T011109
ISS off Degraded spatial resolution & polarimetric sensitivity
243080673
20220308T011209
ISS off Degraded spatial resolution & polarimetric sensitivity
243080674
20220308T011309
ISS off Degraded spatial resolution & polarimetric sensitivity
243080675
20220308T011409
ISS off Degraded spatial resolution & polarimetric sensitivity
243080676
20220308T011509
ISS off Degraded spatial resolution & polarimetric sensitivity
243080677
20220308T011609
ISS off Degraded spatial resolution & polarimetric sensitivity
243080678
20220308T011709
ISS off Degraded spatial resolution & polarimetric sensitivity
243080679
20220308T011809
ISS off Degraded spatial resolution & polarimetric sensitivity
243080680
20220308T011909
ISS off Degraded spatial resolution & polarimetric sensitivity
243080681
20220308T012009
ISS off Degraded spatial resolution & polarimetric sensitivity
243080682
20220308T012109
ISS off Degraded spatial resolution & polarimetric sensitivity
243080683
20220308T012209
ISS off Degraded spatial resolution & polarimetric sensitivity
243080684
20220308T012309
ISS off Degraded spatial resolution & polarimetric sensitivity
243080685
20220308T012409
ISS off Degraded spatial resolution & polarimetric sensitivity
243080686
20220308T012509
ISS off Degraded spatial resolution & polarimetric sensitivity
243080687
20220308T012609
ISS off Degraded spatial resolution & polarimetric sensitivity
243080688
20220308T012709
ISS off Degraded spatial resolution & polarimetric sensitivity
243080689
20220308T012809
ISS off Degraded spatial resolution & polarimetric sensitivity
243080690
20220308T012909
ISS off Degraded spatial resolution & polarimetric sensitivity
243080691
20220308T013009
ISS off Degraded spatial resolution & polarimetric sensitivity
243080692
20220308T013109
ISS off Degraded spatial resolution & polarimetric sensitivity
243080693
20220308T013209
ISS off Degraded spatial resolution & polarimetric sensitivity
243080694
20220308T013309
ISS off Degraded spatial resolution & polarimetric sensitivity
243080695
20220308T013409
ISS off Degraded spatial resolution & polarimetric sensitivity
243080696
20220308T013509
ISS off Degraded spatial resolution & polarimetric sensitivity
243080697
20220308T013609
ISS off Degraded spatial resolution & polarimetric sensitivity
243080698
20220308T013709
ISS off Degraded spatial resolution & polarimetric sensitivity
243080699
20220308T013809
ISS off Degraded spatial resolution & polarimetric sensitivity
243080700
20220308T013909
ISS off Degraded spatial resolution & polarimetric sensitivity
243080701
20220308T014009
ISS off Degraded spatial resolution & polarimetric sensitivity
243080702
20220308T014109
ISS off Degraded spatial resolution & polarimetric sensitivity
243080703
20220308T014209
ISS off Degraded spatial resolution & polarimetric sensitivity
243080704
20220308T014309
ISS off Degraded spatial resolution & polarimetric sensitivity
243080705
20220308T014409
ISS off Degraded spatial resolution & polarimetric sensitivity
243080706
20220308T014509
ISS off Degraded spatial resolution & polarimetric sensitivity
243080707
20220308T014609
ISS off Degraded spatial resolution & polarimetric sensitivity
243080708
20220308T014709
ISS off Degraded spatial resolution & polarimetric sensitivity
243080709
20220308T014809
ISS off Degraded spatial resolution & polarimetric sensitivity
243080710
20220308T014909
ISS off Degraded spatial resolution & polarimetric sensitivity
243080711
20220308T015009
ISS off Degraded spatial resolution & polarimetric sensitivity
243080712
20220308T015109
ISS off Degraded spatial resolution & polarimetric sensitivity
243080713
20220308T015209
ISS off Degraded spatial resolution & polarimetric sensitivity
243080714
20220308T015309
ISS off Degraded spatial resolution & polarimetric sensitivity
243080715
20220308T015409
ISS off Degraded spatial resolution & polarimetric sensitivity
243080716
20220308T015509
ISS off Degraded spatial resolution & polarimetric sensitivity
243080717
20220308T015609
ISS off Degraded spatial resolution & polarimetric sensitivity
243080718
20220308T015709
ISS off Degraded spatial resolution & polarimetric sensitivity
243080719
20220308T015809
ISS off Degraded spatial resolution & polarimetric sensitivity
243080720
20220308T015909
ISS off Degraded spatial resolution & polarimetric sensitivity
243170601
20220317T001809
ISS off Degraded spatial resolution & polarimetric sensitivity
243170602
20220317T001909
ISS off Degraded spatial resolution & polarimetric sensitivity
243170603
20220317T002009
ISS off Degraded spatial resolution & polarimetric sensitivity
243170604
20220317T002109
ISS off Degraded spatial resolution & polarimetric sensitivity
243170605
20220317T002209
ISS off Degraded spatial resolution & polarimetric sensitivity
243170606
20220317T002309
ISS off Degraded spatial resolution & polarimetric sensitivity
243170607
20220317T002409
ISS off Degraded spatial resolution & polarimetric sensitivity
243170608
20220317T002509
ISS off Degraded spatial resolution & polarimetric sensitivity
243170609
20220317T002609
ISS off Degraded spatial resolution & polarimetric sensitivity
243170610
20220317T002709
ISS off Degraded spatial resolution & polarimetric sensitivity
243170611
20220317T002809
ISS off Degraded spatial resolution & polarimetric sensitivity
243170612
20220317T002909
ISS off Degraded spatial resolution & polarimetric sensitivity
243170613
20220317T003009
ISS off Degraded spatial resolution & polarimetric sensitivity
243170614
20220317T003109
ISS off Degraded spatial resolution & polarimetric sensitivity
243170615
20220317T003209
ISS off Degraded spatial resolution & polarimetric sensitivity
243170616
20220317T003309
ISS off Degraded spatial resolution & polarimetric sensitivity
243170617
20220317T003409
ISS off Degraded spatial resolution & polarimetric sensitivity
243170618
20220317T003509
ISS off Degraded spatial resolution & polarimetric sensitivity
243170619
20220317T003609
ISS off Degraded spatial resolution & polarimetric sensitivity
243170620
20220317T003709
ISS off Degraded spatial resolution & polarimetric sensitivity
243170621
20220317T003809
ISS off Degraded spatial resolution & polarimetric sensitivity
243170622
20220317T003909
ISS off Degraded spatial resolution & polarimetric sensitivity
243170623
20220317T004009
ISS off Degraded spatial resolution & polarimetric sensitivity
243170624
20220317T004109
ISS off Degraded spatial resolution & polarimetric sensitivity
243170625
20220317T004209
ISS off Degraded spatial resolution & polarimetric sensitivity
243170626
20220317T004309
ISS off Degraded spatial resolution & polarimetric sensitivity
243170627
20220317T004409
ISS off Degraded spatial resolution & polarimetric sensitivity
243170628
20220317T004509
ISS off Degraded spatial resolution & polarimetric sensitivity
243170629
20220317T004609
ISS off Degraded spatial resolution & polarimetric sensitivity
243170630
20220317T004709
ISS off Degraded spatial resolution & polarimetric sensitivity
243170201
20220317T031809
ISS off Degraded spatial resolution & polarimetric sensitivity
243170202
20220317T031909
ISS off Degraded spatial resolution & polarimetric sensitivity
243170203
20220317T032009
ISS off Degraded spatial resolution & polarimetric sensitivity
243170204
20220317T032109
ISS off Degraded spatial resolution & polarimetric sensitivity
243170205
20220317T032209
ISS off Degraded spatial resolution & polarimetric sensitivity
243170206
20220317T032309
ISS off Degraded spatial resolution & polarimetric sensitivity
243170207
20220317T032409
ISS off Degraded spatial resolution & polarimetric sensitivity
243170208
20220317T032509
ISS off Degraded spatial resolution & polarimetric sensitivity
243170210
20220317T032709
ISS off Degraded spatial resolution & polarimetric sensitivity
243170211
20220317T032809
ISS off Degraded spatial resolution & polarimetric sensitivity
243170212
20220317T032909
ISS off Degraded spatial resolution & polarimetric sensitivity
243170213
20220317T033009
ISS off Degraded spatial resolution & polarimetric sensitivity
243170214
20220317T033109
ISS off Degraded spatial resolution & polarimetric sensitivity
243170215
20220317T033209
ISS off Degraded spatial resolution & polarimetric sensitivity
243170216
20220317T033309
ISS off Degraded spatial resolution & polarimetric sensitivity
243170217
20220317T033409
ISS off Degraded spatial resolution & polarimetric sensitivity
243170218
20220317T033509
ISS off Degraded spatial resolution & polarimetric sensitivity
243170219
20220317T033609
ISS off Degraded spatial resolution & polarimetric sensitivity
243170220
20220317T033709
ISS off Degraded spatial resolution & polarimetric sensitivity
243170221
20220317T033809
ISS off Degraded spatial resolution & polarimetric sensitivity
243170222
20220317T033909
ISS off Degraded spatial resolution & polarimetric sensitivity
243170223
20220317T034009
ISS off Degraded spatial resolution & polarimetric sensitivity
243170224
20220317T034109
ISS off Degraded spatial resolution & polarimetric sensitivity
243170225
20220317T034209
ISS off Degraded spatial resolution & polarimetric sensitivity
243170226
20220317T034309
ISS off Degraded spatial resolution & polarimetric sensitivity
243170227
20220317T034409
ISS off Degraded spatial resolution & polarimetric sensitivity
243170228
20220317T034509
ISS off Degraded spatial resolution & polarimetric sensitivity
243170229
20220317T034609
ISS off Degraded spatial resolution & polarimetric sensitivity
243170230
20220317T034709
ISS off Degraded spatial resolution & polarimetric sensitivity
243180101
20220318T101009
ISS off Degraded spatial resolution & polarimetric sensitivity
243180102
20220318T101509
ISS off Degraded spatial resolution & polarimetric sensitivity
243180103
20220318T102009
ISS off Degraded spatial resolution & polarimetric sensitivity
243180104
20220318T102509
ISS off Degraded spatial resolution & polarimetric sensitivity
243180105
20220318T103009
ISS off Degraded spatial resolution & polarimetric sensitivity
243180106
20220318T103509
ISS off Degraded spatial resolution & polarimetric sensitivity
243180107
20220318T104009
ISS off Degraded spatial resolution & polarimetric sensitivity
243180108
20220318T104509
ISS off Degraded spatial resolution & polarimetric sensitivity
243180109
20220318T105009
ISS off Degraded spatial resolution & polarimetric sensitivity
243180110
20220318T105509
ISS off Degraded spatial resolution & polarimetric sensitivity
243180111
20220318T110009
ISS off Degraded spatial resolution & polarimetric sensitivity
243180112
20220318T110509
ISS off Degraded spatial resolution & polarimetric sensitivity
243190101
20220319T103609
ISS off Degraded spatial resolution & polarimetric sensitivity
243190102
20220319T104109
ISS off Degraded spatial resolution & polarimetric sensitivity
243190103
20220319T104609
ISS off Degraded spatial resolution & polarimetric sensitivity
243190104
20220319T105109
ISS off Degraded spatial resolution & polarimetric sensitivity
243190105
20220319T105609
ISS off Degraded spatial resolution & polarimetric sensitivity
243190106
20220319T110109
ISS off Degraded spatial resolution & polarimetric sensitivity
243190107
20220319T110609
ISS off Degraded spatial resolution & polarimetric sensitivity
243190108
20220319T111109
ISS off Degraded spatial resolution & polarimetric sensitivity
243190109
20220319T111609
ISS off Degraded spatial resolution & polarimetric sensitivity
243190110
20220319T112109
ISS off Degraded spatial resolution & polarimetric sensitivity
243190111
20220319T112609
ISS off Degraded spatial resolution & polarimetric sensitivity
243190112
20220319T113109
ISS off Degraded spatial resolution & polarimetric sensitivity
243200101
20220320T112709
ISS off Degraded spatial resolution & polarimetric sensitivity
243200102
20220320T113209
ISS off Degraded spatial resolution & polarimetric sensitivity
243200103
20220320T113709
ISS off Degraded spatial resolution & polarimetric sensitivity
243200104
20220320T114209
ISS off Degraded spatial resolution & polarimetric sensitivity
243200105
20220320T114709
ISS off Degraded spatial resolution & polarimetric sensitivity
243200106
20220320T115209
ISS off Degraded spatial resolution & polarimetric sensitivity
243200107
20220320T115709
ISS off Degraded spatial resolution & polarimetric sensitivity
243200108
20220320T120209
ISS off Degraded spatial resolution & polarimetric sensitivity
243200109
20220320T120709
ISS off Degraded spatial resolution & polarimetric sensitivity
243200110
20220320T121209
ISS off Degraded spatial resolution & polarimetric sensitivity
243200111
20220320T121709
ISS off Degraded spatial resolution & polarimetric sensitivity
243200112
20220320T122209
ISS off Degraded spatial resolution & polarimetric sensitivity
243210101
20220321T113609
ISS off Degraded spatial resolution & polarimetric sensitivity
243210102
20220321T114109
ISS off Degraded spatial resolution & polarimetric sensitivity
243210103
20220321T114609
ISS off Degraded spatial resolution & polarimetric sensitivity
243210104
20220321T115109
ISS off Degraded spatial resolution & polarimetric sensitivity
243210105
20220321T115609
ISS off Degraded spatial resolution & polarimetric sensitivity
243210106
20220321T120109
ISS off Degraded spatial resolution & polarimetric sensitivity
243210107
20220321T120609
ISS off Degraded spatial resolution & polarimetric sensitivity
243210108
20220321T121109
ISS off Degraded spatial resolution & polarimetric sensitivity
243210109
20220321T121609
ISS off Degraded spatial resolution & polarimetric sensitivity
243210110
20220321T122109
ISS off Degraded spatial resolution & polarimetric sensitivity
243210111
20220321T122609
ISS off Degraded spatial resolution & polarimetric sensitivity
243210112
20220321T123109
ISS off Degraded spatial resolution & polarimetric sensitivity
243220101
20220322T094009
ISS off Degraded spatial resolution & polarimetric sensitivity
243220102
20220322T094149
ISS off Degraded spatial resolution & polarimetric sensitivity
243220103
20220322T094329
ISS off Degraded spatial resolution & polarimetric sensitivity
243220104
20220322T094509
ISS off Degraded spatial resolution & polarimetric sensitivity
243220105
20220322T094649
ISS off Degraded spatial resolution & polarimetric sensitivity
243220106
20220322T094829
ISS off Degraded spatial resolution & polarimetric sensitivity
243220107
20220322T095009
ISS off Degraded spatial resolution & polarimetric sensitivity
243220108
20220322T095149
ISS off Degraded spatial resolution & polarimetric sensitivity
243220109
20220322T095329
ISS off Degraded spatial resolution & polarimetric sensitivity
243220110
20220322T095509
ISS off Degraded spatial resolution & polarimetric sensitivity
243220111
20220322T095649
ISS off Degraded spatial resolution & polarimetric sensitivity
243220112
20220322T095829
ISS off Degraded spatial resolution & polarimetric sensitivity
243220113
20220322T100009
ISS off Degraded spatial resolution & polarimetric sensitivity
243220114
20220322T100149
ISS off Degraded spatial resolution & polarimetric sensitivity
243220115
20220322T100329
ISS off Degraded spatial resolution & polarimetric sensitivity
243220116
20220322T100509
ISS off Degraded spatial resolution & polarimetric sensitivity
243220117
20220322T100649
ISS off Degraded spatial resolution & polarimetric sensitivity
243220118
20220322T100829
ISS off Degraded spatial resolution & polarimetric sensitivity
243220119
20220322T101009
ISS off Degraded spatial resolution & polarimetric sensitivity
243220120
20220322T101149
ISS off Degraded spatial resolution & polarimetric sensitivity
243220121
20220322T101329
ISS off Degraded spatial resolution & polarimetric sensitivity
243220122
20220322T101509
ISS off Degraded spatial resolution & polarimetric sensitivity
243220123
20220322T101649
ISS off Degraded spatial resolution & polarimetric sensitivity
243220124
20220322T101829
ISS off Degraded spatial resolution & polarimetric sensitivity
243220125
20220322T102009
ISS off Degraded spatial resolution & polarimetric sensitivity
243220126
20220322T102149
ISS off Degraded spatial resolution & polarimetric sensitivity
243220127
20220322T102329
ISS off Degraded spatial resolution & polarimetric sensitivity
243300101
20220330T001809
ISS off
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
V_LOS not released due to remaining artefacts
243300102
20220330T001949
ISS off
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
V_LOS not released due to remaining artefacts
243300103
20220330T002128
ISS off
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
V_LOS not released due to remaining artefacts
243300104
20220330T002309
ISS off
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
V_LOS not released due to remaining artefacts
243300105
20220330T002448
ISS off
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
V_LOS not released due to remaining artefacts
243300106
20220330T002628
ISS off
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
V_LOS not released due to remaining artefacts
243300107
20220330T002808
ISS off
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
V_LOS not released due to remaining artefacts
243300108
20220330T002948
ISS off
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
V_LOS not released due to remaining artefacts
243300109
20220330T003128
ISS off
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
V_LOS not released due to remaining artefacts
243300111
20220330T003448
ISS off
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
V_LOS not released due to remaining artefacts
243300112
20220330T003628
ISS off
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
V_LOS not released due to remaining artefacts
243300113
20220330T003809
ISS off
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
V_LOS not released due to remaining artefacts
243300115
20220330T004129
ISS off
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
V_LOS not released due to remaining artefacts
243300116
20220330T004309
ISS off
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
V_LOS not released due to remaining artefacts
243300117
20220330T004448
ISS off
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
V_LOS not released due to remaining artefacts
243300118
20220330T004628
ISS off
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
V_LOS not released due to remaining artefacts
243300701
20220330T033009
ISS off Degraded spatial resolution & polarimetric sensitivity
243300702
20220330T033219
ISS off Degraded spatial resolution & polarimetric sensitivity
243300703
20220330T033429
ISS off Degraded spatial resolution & polarimetric sensitivity
243300704
20220330T033639
ISS off Degraded spatial resolution & polarimetric sensitivity
243300705
20220330T033849
ISS off Degraded spatial resolution & polarimetric sensitivity
243300706
20220330T034059
ISS off Degraded spatial resolution & polarimetric sensitivity
243300707
20220330T034309
ISS off Degraded spatial resolution & polarimetric sensitivity
243300708
20220330T034519
ISS off Degraded spatial resolution & polarimetric sensitivity
243300709
20220330T034729
ISS off Degraded spatial resolution & polarimetric sensitivity
243300710
20220330T034939
ISS off Degraded spatial resolution & polarimetric sensitivity
243300711
20220330T035149
ISS off Degraded spatial resolution & polarimetric sensitivity
243300712
20220330T035359
ISS off Degraded spatial resolution & polarimetric sensitivity
243300713
20220330T035609
ISS off Degraded spatial resolution & polarimetric sensitivity
243300714
20220330T035819
ISS off Degraded spatial resolution & polarimetric sensitivity
243300715
20220330T040029
ISS off Degraded spatial resolution & polarimetric sensitivity
243300716
20220330T040239
ISS off Degraded spatial resolution & polarimetric sensitivity
243300717
20220330T040449
ISS off Degraded spatial resolution & polarimetric sensitivity
243300719
20220330T040909
ISS off Degraded spatial resolution & polarimetric sensitivity
243300720
20220330T041119
ISS off Degraded spatial resolution & polarimetric sensitivity
243300721
20220330T041329
ISS off Degraded spatial resolution & polarimetric sensitivity
243300722
20220330T041539
ISS off Degraded spatial resolution & polarimetric sensitivity
243300723
20220330T041749
ISS off Degraded spatial resolution & polarimetric sensitivity
243300724
20220330T041959
ISS off Degraded spatial resolution & polarimetric sensitivity
243300725
20220330T042209
ISS off Degraded spatial resolution & polarimetric sensitivity
243300726
20220330T042419
ISS off Degraded spatial resolution & polarimetric sensitivity
243300727
20220330T042629
ISS off Degraded spatial resolution & polarimetric sensitivity
243300728
20220330T042839
ISS off Degraded spatial resolution & polarimetric sensitivity
243300729
20220330T043049
ISS off Degraded spatial resolution & polarimetric sensitivity
243300730
20220330T043259
ISS off Degraded spatial resolution & polarimetric sensitivity
243300731
20220330T043509
ISS off Degraded spatial resolution & polarimetric sensitivity
243300732
20220330T043719
ISS off Degraded spatial resolution & polarimetric sensitivity
243300733
20220330T044009
ISS off Degraded spatial resolution & polarimetric sensitivity
243300734
20220330T044149
ISS off Degraded spatial resolution & polarimetric sensitivity
243300735
20220330T044329
ISS off Degraded spatial resolution & polarimetric sensitivity
243300736
20220330T044509
ISS off Degraded spatial resolution & polarimetric sensitivity
243300737
20220330T044649
ISS off Degraded spatial resolution & polarimetric sensitivity
243300738
20220330T044829
ISS off Degraded spatial resolution & polarimetric sensitivity
243300739
20220330T045009
ISS off Degraded spatial resolution & polarimetric sensitivity
243300740
20220330T045149
ISS off Degraded spatial resolution & polarimetric sensitivity
243300741
20220330T045329
ISS off Degraded spatial resolution & polarimetric sensitivity
243300742
20220330T045509
ISS off Degraded spatial resolution & polarimetric sensitivity
243300743
20220330T045649
ISS off Degraded spatial resolution & polarimetric sensitivity
243300744
20220330T045829
ISS off Degraded spatial resolution & polarimetric sensitivity
243300745
20220330T050009
ISS off Degraded spatial resolution & polarimetric sensitivity
243300301
20220330T090003
ISS off Degraded spatial resolution & polarimetric sensitivity
243300302
20220330T102003
ISS off Degraded spatial resolution & polarimetric sensitivity
243300303
20220330T114003
ISS off Degraded spatial resolution & polarimetric sensitivity
243300304
20220330T130003
ISS off Degraded spatial resolution & polarimetric sensitivity
243300305
20220330T142003
ISS off Degraded spatial resolution & polarimetric sensitivity
243300307
20220330T170003
ISS off Degraded spatial resolution & polarimetric sensitivity
243300308
20220330T182003
ISS off Degraded spatial resolution & polarimetric sensitivity
243300310
20220330T210003
ISS off Degraded spatial resolution & polarimetric sensitivity
243300311
20220330T222003
ISS off Degraded spatial resolution & polarimetric sensitivity
243300312
20220330T234003
ISS off Degraded spatial resolution & polarimetric sensitivity
243310301
20220331T035003
ISS off Degraded spatial resolution & polarimetric sensitivity
243310302
20220331T051003
ISS off Degraded spatial resolution & polarimetric sensitivity
243310303
20220331T063003
ISS off Degraded spatial resolution & polarimetric sensitivity
243310304
20220331T075003
ISS off Degraded spatial resolution & polarimetric sensitivity
243310305
20220331T091003
ISS off Degraded spatial resolution & polarimetric sensitivity
243310306
20220331T103003
ISS off Degraded spatial resolution & polarimetric sensitivity
243310307
20220331T115003
ISS off Degraded spatial resolution & polarimetric sensitivity
243310308
20220331T130503
ISS off Degraded spatial resolution & polarimetric sensitivity
243310309
20220331T143003
ISS off Degraded spatial resolution & polarimetric sensitivity
243310310
20220331T155003
ISS off Degraded spatial resolution & polarimetric sensitivity
243310311
20220331T171003
ISS off Degraded spatial resolution & polarimetric sensitivity
243310801
20220331T175603
ISS off Degraded spatial resolution & polarimetric sensitivity
243310802
20220331T182609
ISS off Degraded spatial resolution & polarimetric sensitivity
243310803
20220331T185609
ISS off Degraded spatial resolution & polarimetric sensitivity
243310804
20220331T192609
ISS off Degraded spatial resolution & polarimetric sensitivity
243310805
20220331T195608
ISS off Degraded spatial resolution & polarimetric sensitivity
243310806
20220331T202608
ISS off Degraded spatial resolution & polarimetric sensitivity
243310807
20220331T205603
ISS off Degraded spatial resolution & polarimetric sensitivity
243310808
20220331T212609
ISS off Degraded spatial resolution & polarimetric sensitivity
243310809
20220331T215609
ISS off Degraded spatial resolution & polarimetric sensitivity
243310810
20220331T222609
ISS off Degraded spatial resolution & polarimetric sensitivity
243310811
20220331T225609
ISS off Degraded spatial resolution & polarimetric sensitivity
243310812
20220331T232609
ISS off Degraded spatial resolution & polarimetric sensitivity
243310813
20220331T235609
ISS off Degraded spatial resolution & polarimetric sensitivity
244010801
20220401T002603
ISS off Degraded spatial resolution & polarimetric sensitivity
244010802
20220401T005610
ISS off Degraded spatial resolution & polarimetric sensitivity
244010803
20220401T012610
ISS off Degraded spatial resolution & polarimetric sensitivity
244010804
20220401T015610
ISS off Degraded spatial resolution & polarimetric sensitivity
244010805
20220401T022610
ISS off Degraded spatial resolution & polarimetric sensitivity
244010806
20220401T025609
ISS off Degraded spatial resolution & polarimetric sensitivity
244010807
20220401T032603
ISS off Degraded spatial resolution & polarimetric sensitivity
244010808
20220401T035609
ISS off Degraded spatial resolution & polarimetric sensitivity
244010809
20220401T042609
ISS off Degraded spatial resolution & polarimetric sensitivity
244010810
20220401T045609
ISS off Degraded spatial resolution & polarimetric sensitivity
244010811
20220401T052609
ISS off Degraded spatial resolution & polarimetric sensitivity
244010812
20220401T055609
ISS off Degraded spatial resolution & polarimetric sensitivity
244010813
20220401T062603
ISS off Degraded spatial resolution & polarimetric sensitivity
244010814
20220401T065609
ISS off Degraded spatial resolution & polarimetric sensitivity
244010815
20220401T072609
ISS off Degraded spatial resolution & polarimetric sensitivity
244010816
20220401T075609
ISS off Degraded spatial resolution & polarimetric sensitivity
244010817
20220401T082609
ISS off Degraded spatial resolution & polarimetric sensitivity
244010818
20220401T085609
ISS off Degraded spatial resolution & polarimetric sensitivity
244010819
20220401T092603
ISS off Degraded spatial resolution & polarimetric sensitivity
244010820
20220401T095609
ISS off Degraded spatial resolution & polarimetric sensitivity
244010821
20220401T102609
ISS off Degraded spatial resolution & polarimetric sensitivity
244010822
20220401T105609
ISS off Degraded spatial resolution & polarimetric sensitivity
244010823
20220401T112609
ISS off Degraded spatial resolution & polarimetric sensitivity
244010824
20220401T115609
ISS off Degraded spatial resolution & polarimetric sensitivity
244010825
20220401T122603
ISS off Degraded spatial resolution & polarimetric sensitivity
244010826
20220401T125609
ISS off Degraded spatial resolution & polarimetric sensitivity
244010827
20220401T132609
ISS off Degraded spatial resolution & polarimetric sensitivity
244010828
20220401T135609
ISS off Degraded spatial resolution & polarimetric sensitivity
244010829
20220401T142609
ISS off Degraded spatial resolution & polarimetric sensitivity
244010830
20220401T145609
ISS off Degraded spatial resolution & polarimetric sensitivity
244010831
20220401T152603
ISS off Degraded spatial resolution & polarimetric sensitivity
244010832
20220401T155609
ISS off Degraded spatial resolution & polarimetric sensitivity
244010833
20220401T162609
ISS off Degraded spatial resolution & polarimetric sensitivity
244010834
20220401T165609
ISS off Degraded spatial resolution & polarimetric sensitivity
244010835
20220401T172609
ISS off Degraded spatial resolution & polarimetric sensitivity
244010836
20220401T175609
ISS off Degraded spatial resolution & polarimetric sensitivity
244010837
20220401T182603
ISS off Degraded spatial resolution & polarimetric sensitivity
244010838
20220401T185609
ISS off Degraded spatial resolution & polarimetric sensitivity
244010839
20220401T192609
ISS off Degraded spatial resolution & polarimetric sensitivity
244010840
20220401T195609
ISS off Degraded spatial resolution & polarimetric sensitivity
244010841
20220401T202609
ISS off Degraded spatial resolution & polarimetric sensitivity
244010842
20220401T205609
ISS off Degraded spatial resolution & polarimetric sensitivity
244010843
20220401T212603
ISS off Degraded spatial resolution & polarimetric sensitivity
244010844
20220401T215609
ISS off Degraded spatial resolution & polarimetric sensitivity
244010845
20220401T222609
ISS off Degraded spatial resolution & polarimetric sensitivity
244010846
20220401T225609
ISS off Degraded spatial resolution & polarimetric sensitivity
244010847
20220401T232609
ISS off Degraded spatial resolution & polarimetric sensitivity
244010848
20220401T235609
ISS off Degraded spatial resolution & polarimetric sensitivity
244020801
20220402T032604
ISS off Degraded spatial resolution & polarimetric sensitivity
244020802
20220402T035610
ISS off Degraded spatial resolution & polarimetric sensitivity
244020803
20220402T042610
ISS off Degraded spatial resolution & polarimetric sensitivity
244020804
20220402T045609
ISS off Degraded spatial resolution & polarimetric sensitivity
244020805
20220402T052609
ISS off Degraded spatial resolution & polarimetric sensitivity
244020806
20220402T055609
ISS off Degraded spatial resolution & polarimetric sensitivity
244020807
20220402T062603
ISS off Degraded spatial resolution & polarimetric sensitivity
244020808
20220402T065609
ISS off Degraded spatial resolution & polarimetric sensitivity
244020809
20220402T072609
ISS off Degraded spatial resolution & polarimetric sensitivity
244020810
20220402T075609
ISS off Degraded spatial resolution & polarimetric sensitivity
244020811
20220402T082609
ISS off Degraded spatial resolution & polarimetric sensitivity
244020812
20220402T085609
ISS off Degraded spatial resolution & polarimetric sensitivity
244020813
20220402T092604
ISS off Degraded spatial resolution & polarimetric sensitivity
244020814
20220402T095610
ISS off Degraded spatial resolution & polarimetric sensitivity
244020815
20220402T102609
ISS off Degraded spatial resolution & polarimetric sensitivity
244020816
20220402T105609
ISS off Degraded spatial resolution & polarimetric sensitivity
244020817
20220402T112609
ISS off Degraded spatial resolution & polarimetric sensitivity
244020818
20220402T115609
ISS off Degraded spatial resolution & polarimetric sensitivity
244020819
20220402T122603
ISS off Degraded spatial resolution & polarimetric sensitivity
244020820
20220402T125609
ISS off Degraded spatial resolution & polarimetric sensitivity
244020821
20220402T132609
ISS off Degraded spatial resolution & polarimetric sensitivity
244020822
20220402T135609
ISS off Degraded spatial resolution & polarimetric sensitivity
244020823
20220402T142609
ISS off Degraded spatial resolution & polarimetric sensitivity
244020824
20220402T145609
ISS off Degraded spatial resolution & polarimetric sensitivity
244020825
20220402T152603
ISS off Degraded spatial resolution & polarimetric sensitivity
244020826
20220402T155609
ISS off Degraded spatial resolution & polarimetric sensitivity
244020827
20220402T162609
ISS off Degraded spatial resolution & polarimetric sensitivity
244020828
20220402T165609
ISS off Degraded spatial resolution & polarimetric sensitivity
244020829
20220402T172609
ISS off Degraded spatial resolution & polarimetric sensitivity
244020830
20220402T175609
ISS off Degraded spatial resolution & polarimetric sensitivity
244020831
20220402T182603
ISS off Degraded spatial resolution & polarimetric sensitivity
244020832
20220402T185609
ISS off Degraded spatial resolution & polarimetric sensitivity
244020833
20220402T192609
ISS off Degraded spatial resolution & polarimetric sensitivity
244020834
20220402T195609
ISS off Degraded spatial resolution & polarimetric sensitivity
244020835
20220402T202609
ISS off Degraded spatial resolution & polarimetric sensitivity
244020836
20220402T205609
ISS off Degraded spatial resolution & polarimetric sensitivity
244020837
20220402T212603
ISS off Degraded spatial resolution & polarimetric sensitivity
244020838
20220402T215609
ISS off Degraded spatial resolution & polarimetric sensitivity
244020839
20220402T222609
ISS off Degraded spatial resolution & polarimetric sensitivity
244020840
20220402T225609
ISS off Degraded spatial resolution & polarimetric sensitivity
244020841
20220402T232609
ISS off Degraded spatial resolution & polarimetric sensitivity
244020842
20220402T235609
ISS off Degraded spatial resolution & polarimetric sensitivity
244030801
20220403T002603
ISS off Degraded spatial resolution & polarimetric sensitivity
244030802
20220403T005609
ISS off Degraded spatial resolution & polarimetric sensitivity
244030803
20220403T012609
ISS off Degraded spatial resolution & polarimetric sensitivity
244030804
20220403T015609
ISS off Degraded spatial resolution & polarimetric sensitivity
244030805
20220403T022609
ISS off Degraded spatial resolution & polarimetric sensitivity
244030806
20220403T025609
ISS off Degraded spatial resolution & polarimetric sensitivity
244030807
20220403T032603
ISS off Degraded spatial resolution & polarimetric sensitivity
244030808
20220403T035609
ISS off Degraded spatial resolution & polarimetric sensitivity
244030809
20220403T042609
ISS off Degraded spatial resolution & polarimetric sensitivity
244030810
20220403T045609
ISS off Degraded spatial resolution & polarimetric sensitivity
244030811
20220403T052609
ISS off Degraded spatial resolution & polarimetric sensitivity
244030812
20220403T055609
ISS off Degraded spatial resolution & polarimetric sensitivity
244030813
20220403T062603
ISS off Degraded spatial resolution & polarimetric sensitivity
244030814
20220403T065609
ISS off Degraded spatial resolution & polarimetric sensitivity
244030815
20220403T072609
ISS off Degraded spatial resolution & polarimetric sensitivity
244030816
20220403T075609
ISS off Degraded spatial resolution & polarimetric sensitivity
244030817
20220403T082609
ISS off Degraded spatial resolution & polarimetric sensitivity
244030818
20220403T085609
ISS off Degraded spatial resolution & polarimetric sensitivity
244030819
20220403T092603
ISS off Degraded spatial resolution & polarimetric sensitivity
244030820
20220403T095609
ISS off Degraded spatial resolution & polarimetric sensitivity
244030821
20220403T102609
ISS off Degraded spatial resolution & polarimetric sensitivity
244030822
20220403T105609
ISS off Degraded spatial resolution & polarimetric sensitivity
244030823
20220403T112609
ISS off Degraded spatial resolution & polarimetric sensitivity
244030824
20220403T115609
ISS off Degraded spatial resolution & polarimetric sensitivity
244030825
20220403T122603
ISS off Degraded spatial resolution & polarimetric sensitivity
244030826
20220403T125609
ISS off Degraded spatial resolution & polarimetric sensitivity
244030827
20220403T132609
ISS off Degraded spatial resolution & polarimetric sensitivity
244030828
20220403T135609
ISS off Degraded spatial resolution & polarimetric sensitivity
244030829
20220403T142609
ISS off Degraded spatial resolution & polarimetric sensitivity
244030830
20220403T145609
ISS off Degraded spatial resolution & polarimetric sensitivity
244030831
20220403T152603
ISS off Degraded spatial resolution & polarimetric sensitivity
244030832
20220403T155609
ISS off Degraded spatial resolution & polarimetric sensitivity
244030833
20220403T162609
ISS off Degraded spatial resolution & polarimetric sensitivity
244030834
20220403T165609
ISS off Degraded spatial resolution & polarimetric sensitivity
244030835
20220403T172609
ISS off Degraded spatial resolution & polarimetric sensitivity
244030836
20220403T175609
ISS off Degraded spatial resolution & polarimetric sensitivity
244030837
20220403T182603
ISS off Degraded spatial resolution & polarimetric sensitivity
244030838
20220403T185609
ISS off Degraded spatial resolution & polarimetric sensitivity
244030839
20220403T192609
ISS off Degraded spatial resolution & polarimetric sensitivity
244030840
20220403T195609
ISS off Degraded spatial resolution & polarimetric sensitivity
244030841
20220403T202609
ISS off Degraded spatial resolution & polarimetric sensitivity
244030842
20220403T205609
ISS off Degraded spatial resolution & polarimetric sensitivity
244030843
20220403T212603
ISS off Degraded spatial resolution & polarimetric sensitivity
244030844
20220403T215609
ISS off Degraded spatial resolution & polarimetric sensitivity
244030845
20220403T222609
ISS off Degraded spatial resolution & polarimetric sensitivity
244030846
20220403T225609
ISS off Degraded spatial resolution & polarimetric sensitivity
244030847
20220403T232609
ISS off Degraded spatial resolution & polarimetric sensitivity
244030848
20220403T235609
ISS off Degraded spatial resolution & polarimetric sensitivity
244040801
20220404T032603
ISS off Degraded spatial resolution & polarimetric sensitivity
244040802
20220404T035609
ISS off Degraded spatial resolution & polarimetric sensitivity
244040803
20220404T042609
ISS off Degraded spatial resolution & polarimetric sensitivity
244040804
20220404T045609
ISS off Degraded spatial resolution & polarimetric sensitivity
244040805
20220404T052609
ISS off Degraded spatial resolution & polarimetric sensitivity
244040806
20220404T055609
ISS off Degraded spatial resolution & polarimetric sensitivity
244040807
20220404T062603
ISS off Degraded spatial resolution & polarimetric sensitivity
244040808
20220404T065609
ISS off Degraded spatial resolution & polarimetric sensitivity
244040809
20220404T072609
ISS off Degraded spatial resolution & polarimetric sensitivity
244040810
20220404T075609
ISS off Degraded spatial resolution & polarimetric sensitivity
244040811
20220404T082609
ISS off Degraded spatial resolution & polarimetric sensitivity
244040812
20220404T085609
ISS off Degraded spatial resolution & polarimetric sensitivity
244040813
20220404T092603
ISS off Degraded spatial resolution & polarimetric sensitivity
244040814
20220404T095609
ISS off Degraded spatial resolution & polarimetric sensitivity
244040815
20220404T102609
ISS off Degraded spatial resolution & polarimetric sensitivity
244040816
20220404T105609
ISS off Degraded spatial resolution & polarimetric sensitivity
244040817
20220404T112609
ISS off Degraded spatial resolution & polarimetric sensitivity
244040818
20220404T115609
ISS off Degraded spatial resolution & polarimetric sensitivity
244040819
20220404T122602
ISS off Degraded spatial resolution & polarimetric sensitivity
244040820
20220404T125609
ISS off Degraded spatial resolution & polarimetric sensitivity
244040821
20220404T132609
ISS off Degraded spatial resolution & polarimetric sensitivity
244040822
20220404T135609
ISS off Degraded spatial resolution & polarimetric sensitivity
244040823
20220404T142609
ISS off Degraded spatial resolution & polarimetric sensitivity
244040824
20220404T145609
ISS off Degraded spatial resolution & polarimetric sensitivity
244040825
20220404T152602
ISS off Degraded spatial resolution & polarimetric sensitivity
250120601
20221012T041709
ISS off Degraded spatial resolution & polarimetric sensitivity
250120602
20221012T042209
ISS off Degraded spatial resolution & polarimetric sensitivity
250120603
20221012T042709
ISS off Degraded spatial resolution & polarimetric sensitivity
250120604
20221012T043209
ISS off Degraded spatial resolution & polarimetric sensitivity
250120605
20221012T043709
ISS off Degraded spatial resolution & polarimetric sensitivity
250120606
20221012T044209
ISS off Degraded spatial resolution & polarimetric sensitivity
250120607
20221012T044709
ISS off Degraded spatial resolution & polarimetric sensitivity
250120608
20221012T045209
ISS off Degraded spatial resolution & polarimetric sensitivity
250120609
20221012T045709
ISS off Degraded spatial resolution & polarimetric sensitivity
250120610
20221012T050209
ISS off Degraded spatial resolution & polarimetric sensitivity
250120611
20221012T050709
ISS off Degraded spatial resolution & polarimetric sensitivity
250120612
20221012T051209
ISS off Degraded spatial resolution & polarimetric sensitivity
250120613
20221012T051709
ISS off Degraded spatial resolution & polarimetric sensitivity
250120614
20221012T052209
ISS off Degraded spatial resolution & polarimetric sensitivity
250120615
20221012T052709
ISS off Degraded spatial resolution & polarimetric sensitivity
250120616
20221012T053209
ISS off Degraded spatial resolution & polarimetric sensitivity
250120617
20221012T053709
ISS off Degraded spatial resolution & polarimetric sensitivity
250120618
20221012T054209
ISS off Degraded spatial resolution & polarimetric sensitivity
250120619
20221012T054709
ISS off Degraded spatial resolution & polarimetric sensitivity
250120620
20221012T055209
ISS off Degraded spatial resolution & polarimetric sensitivity
250120621
20221012T055709
ISS off Degraded spatial resolution & polarimetric sensitivity
250120622
20221012T060209
ISS off Degraded spatial resolution & polarimetric sensitivity
250120623
20221012T060709
ISS off Degraded spatial resolution & polarimetric sensitivity
250120624
20221012T061209
ISS off Degraded spatial resolution & polarimetric sensitivity
250120625
20221012T061709
ISS off Degraded spatial resolution & polarimetric sensitivity
250120626
20221012T062209
ISS off Degraded spatial resolution & polarimetric sensitivity
250120627
20221012T062709
ISS off Degraded spatial resolution & polarimetric sensitivity
250120628
20221012T063209
ISS off Degraded spatial resolution & polarimetric sensitivity
250120629
20221012T063709
ISS off Degraded spatial resolution & polarimetric sensitivity
250120630
20221012T064209
ISS off Degraded spatial resolution & polarimetric sensitivity
250120631
20221012T064709
ISS off Degraded spatial resolution & polarimetric sensitivity
250120632
20221012T065209
ISS off Degraded spatial resolution & polarimetric sensitivity
250120633
20221012T065709
ISS off Degraded spatial resolution & polarimetric sensitivity
250120634
20221012T070209
ISS off Degraded spatial resolution & polarimetric sensitivity
250120635
20221012T070709
ISS off Degraded spatial resolution & polarimetric sensitivity
250120636
20221012T071209
ISS off Degraded spatial resolution & polarimetric sensitivity
250130101
20221013T122109
ISS off Degraded spatial resolution & polarimetric sensitivity
250130102
20221013T122609
ISS off Degraded spatial resolution & polarimetric sensitivity
250130103
20221013T123109
ISS off Degraded spatial resolution & polarimetric sensitivity
250130104
20221013T123609
ISS off Degraded spatial resolution & polarimetric sensitivity
250130105
20221013T124109
ISS off Degraded spatial resolution & polarimetric sensitivity
250130106
20221013T124609
ISS off Degraded spatial resolution & polarimetric sensitivity
250130107
20221013T125109
ISS off Degraded spatial resolution & polarimetric sensitivity
250130108
20221013T125609
ISS off Degraded spatial resolution & polarimetric sensitivity
250130109
20221013T130109
ISS off Degraded spatial resolution & polarimetric sensitivity
250130110
20221013T130609
ISS off Degraded spatial resolution & polarimetric sensitivity
250130111
20221013T131109
ISS off Degraded spatial resolution & polarimetric sensitivity
250130112
20221013T131609
ISS off Degraded spatial resolution & polarimetric sensitivity
250130113
20221013T132109
ISS off Degraded spatial resolution & polarimetric sensitivity
250130114
20221013T132249
ISS off Degraded spatial resolution & polarimetric sensitivity
250130115
20221013T132429
ISS off Degraded spatial resolution & polarimetric sensitivity
250130116
20221013T132609
ISS off Degraded spatial resolution & polarimetric sensitivity
250130117
20221013T132749
ISS off Degraded spatial resolution & polarimetric sensitivity
250130118
20221013T132929
ISS off Degraded spatial resolution & polarimetric sensitivity
250130119
20221013T133109
ISS off Degraded spatial resolution & polarimetric sensitivity
250130120
20221013T133249
ISS off Degraded spatial resolution & polarimetric sensitivity
250130121
20221013T133429
ISS off Degraded spatial resolution & polarimetric sensitivity
250130122
20221013T133609
ISS off Degraded spatial resolution & polarimetric sensitivity
250130123
20221013T133749
ISS off Degraded spatial resolution & polarimetric sensitivity
250130124
20221013T133929
ISS off Degraded spatial resolution & polarimetric sensitivity
250130125
20221013T134109
ISS off Degraded spatial resolution & polarimetric sensitivity
250130126
20221013T134249
ISS off Degraded spatial resolution & polarimetric sensitivity
250130127
20221013T134429
ISS off Degraded spatial resolution & polarimetric sensitivity
250130128
20221013T134609
ISS off Degraded spatial resolution & polarimetric sensitivity
250130129
20221013T134749
ISS off Degraded spatial resolution & polarimetric sensitivity
250130130
20221013T134929
ISS off Degraded spatial resolution & polarimetric sensitivity
250130131
20221013T135109
ISS off Degraded spatial resolution & polarimetric sensitivity
250130132
20221013T135249
ISS off Degraded spatial resolution & polarimetric sensitivity
250130133
20221013T135429
ISS off Degraded spatial resolution & polarimetric sensitivity
250130134
20221013T135609
ISS off Degraded spatial resolution & polarimetric sensitivity
250130135
20221013T135749
ISS off Degraded spatial resolution & polarimetric sensitivity
250130136
20221013T135929
ISS off Degraded spatial resolution & polarimetric sensitivity
250130137
20221013T140109
ISS off Degraded spatial resolution & polarimetric sensitivity
250130138
20221013T140249
ISS off Degraded spatial resolution & polarimetric sensitivity
250130139
20221013T140429
ISS off Degraded spatial resolution & polarimetric sensitivity
250130140
20221013T140609
ISS off Degraded spatial resolution & polarimetric sensitivity
250130141
20221013T140749
ISS off Degraded spatial resolution & polarimetric sensitivity
250130142
20221013T140929
ISS off Degraded spatial resolution & polarimetric sensitivity
250130143
20221013T141109
ISS off Degraded spatial resolution & polarimetric sensitivity
250130144
20221013T141249
ISS off Degraded spatial resolution & polarimetric sensitivity
250130145
20221013T141429
ISS off Degraded spatial resolution & polarimetric sensitivity
250130146
20221013T141609
ISS off Degraded spatial resolution & polarimetric sensitivity
250130147
20221013T141749
ISS off Degraded spatial resolution & polarimetric sensitivity
250130148
20221013T141929
ISS off Degraded spatial resolution & polarimetric sensitivity
250130149
20221013T142209
ISS off Degraded spatial resolution & polarimetric sensitivity
250130150
20221013T142709
ISS off Degraded spatial resolution & polarimetric sensitivity
250130151
20221013T143209
ISS off Degraded spatial resolution & polarimetric sensitivity
250130152
20221013T143709
ISS off Degraded spatial resolution & polarimetric sensitivity
250130153
20221013T144209
ISS off Degraded spatial resolution & polarimetric sensitivity
250130154
20221013T144709
ISS off Degraded spatial resolution & polarimetric sensitivity
250130155
20221013T145209
ISS off Degraded spatial resolution & polarimetric sensitivity
250130156
20221013T145709
ISS off Degraded spatial resolution & polarimetric sensitivity
250130157
20221013T150209
ISS off Degraded spatial resolution & polarimetric sensitivity
250130158
20221013T150709
ISS off Degraded spatial resolution & polarimetric sensitivity
250130159
20221013T151209
ISS off Degraded spatial resolution & polarimetric sensitivity
250130160
20221013T151709
ISS off Degraded spatial resolution & polarimetric sensitivity
250130701
20221013T163008
ISS off Degraded spatial resolution & polarimetric sensitivity
250140701
20221014T034009
ISS off Degraded spatial resolution & polarimetric sensitivity
250140702
20221014T135008
ISS off Degraded spatial resolution & polarimetric sensitivity
250140703
20221014T235509
ISS off Degraded spatial resolution & polarimetric sensitivity
250150701
20221015T064008
ISS off Degraded spatial resolution & polarimetric sensitivity
250150702
20221015T135009
ISS off Degraded spatial resolution & polarimetric sensitivity
250160601
20221016T040009
ISS off Degraded spatial resolution & polarimetric sensitivity
250160602
20221016T050009
ISS off Degraded spatial resolution & polarimetric sensitivity
250160603
20221016T060009
ISS off Degraded spatial resolution & polarimetric sensitivity
250160801
20221016T103010
ISS off Degraded spatial resolution & polarimetric sensitivity
250160802
20221016T103240
ISS off Degraded spatial resolution & polarimetric sensitivity
250160803
20221016T103510
ISS off Degraded spatial resolution & polarimetric sensitivity
250160804
20221016T103740
ISS off Degraded spatial resolution & polarimetric sensitivity
250160805
20221016T104010
ISS off Degraded spatial resolution & polarimetric sensitivity
250160806
20221016T104240
ISS off Degraded spatial resolution & polarimetric sensitivity
250160807
20221016T104510
ISS off Degraded spatial resolution & polarimetric sensitivity
250160808
20221016T104740
ISS off Degraded spatial resolution & polarimetric sensitivity
250160809
20221016T105010
ISS off Degraded spatial resolution & polarimetric sensitivity
250160810
20221016T105240
ISS off Degraded spatial resolution & polarimetric sensitivity
250160811
20221016T105510
ISS off Degraded spatial resolution & polarimetric sensitivity
250160812
20221016T105740
ISS off Degraded spatial resolution & polarimetric sensitivity
250160813
20221016T110010
ISS off Degraded spatial resolution & polarimetric sensitivity
250160814
20221016T110240
ISS off Degraded spatial resolution & polarimetric sensitivity
250160815
20221016T110510
ISS off Degraded spatial resolution & polarimetric sensitivity
250160816
20221016T110740
ISS off Degraded spatial resolution & polarimetric sensitivity
250160817
20221016T111010
ISS off Degraded spatial resolution & polarimetric sensitivity
250160818
20221016T111240
ISS off Degraded spatial resolution & polarimetric sensitivity
250160819
20221016T111510
ISS off Degraded spatial resolution & polarimetric sensitivity
250160820
20221016T111740
ISS off Degraded spatial resolution & polarimetric sensitivity
250160821
20221016T112010
ISS off Degraded spatial resolution & polarimetric sensitivity
250160822
20221016T112240
ISS off Degraded spatial resolution & polarimetric sensitivity
250160823
20221016T112510
ISS off Degraded spatial resolution & polarimetric sensitivity
250160824
20221016T112740
ISS off Degraded spatial resolution & polarimetric sensitivity
250170102
20221017T011503
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250170103
20221017T021503
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250170104
20221017T031503
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250170105
20221017T041509
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250170106
20221017T051503
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250170107
20221017T061509
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250170108
20221017T071503
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250170109
20221017T081509
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250170110
20221017T091503
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250170111
20221017T101510
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250170112
20221017T111503
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250170113
20221017T121509
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
2141701114
20221017T131503
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
2141701115
20221017T141509
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250170116
20221017T151503
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250170117
20221017T161509
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250170118
20221017T171503
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250170119
20221017T181509
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250170120
20221017T191503
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250170121
20221017T201503
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250170122
20221017T211503
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250170123
20221017T220403
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250170124
20221017T231503
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250180104
20221018T031503
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250180105
20221018T041503
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250180106
20221018T051509
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250180107
20221018T061503
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250180108
20221018T071510
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250180109
20221018T081503
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250180110
20221018T091509
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250180111
20221018T101503
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250180112
20221018T111509
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250180113
20221018T121503
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250180114
20221018T131509
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250180115
20221018T141503
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250180116
20221018T151509
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250180117
20221018T161503
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250180118
20221018T171509
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250180119
20221018T181503
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250180120
20221018T191503
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250180121
20221018T201503
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250180122
20221018T211503
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250180123
20221018T221509
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250180124
20221018T231502
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250190101
20221019T001502
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250190102
20221019T011503
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250190103
20221019T021509
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250190104
20221019T031503
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250190105
20221019T041509
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250190106
20221019T051503
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250190107
20221019T061509
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250190108
20221019T071503
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250190109
20221019T081509
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250190110
20221019T091503
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250190111
20221019T101509
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250190112
20221019T111503
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250190113
20221019T121509
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250190114
20221019T131503
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250190115
20221019T141509
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250190116
20221019T151503
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250190117
20221019T161509
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250190118
20221019T171503
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250190119
20221019T181509
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250190120
20221019T191503
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250190121
20221019T201503
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250190122
20221019T211503
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250190123
20221019T221509
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250190124
20221019T231502
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250200104
20221020T031502
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250200105
20221020T041503
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250200106
20221020T051509
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250200107
20221020T061503
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250200108
20221020T071510
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250200109
20221020T081503
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250200110
20221020T091509
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250200111
20221020T101503
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250200112
20221020T111509
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250200113
20221020T121503
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250200114
20221020T131509
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250200115
20221020T141503
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250200116
20221020T151509
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250200117
20221020T161503
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250200118
20221020T171509
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250200119
20221020T181503
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250200120
20221020T191502
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250200121
20221020T201502
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250200122
20221020T211503
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250200123
20221020T221509
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250200124
20221020T231502
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250210101
20221021T001502
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250210102
20221021T011503
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250210103
20221021T021509
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250210104
20221021T031503
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250210105
20221021T041509
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250210106
20221021T051503
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250210107
20221021T061509
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250210108
20221021T071503
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250210109
20221021T081509
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250210110
20221021T091503
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250210111
20221021T101509
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250210112
20221021T111503
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250210113
20221021T121509
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250210114
20221021T131503
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250210115
20221021T141509
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250210116
20221021T151503
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250210117
20221021T161510
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250210118
20221021T171503
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250210119
20221021T181509
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250210120
20221021T191503
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250210121
20221021T201502
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250210122
20221021T211503
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250210123
20221021T221509
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250210124
20221021T231502
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250220104
20221022T031502
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250220105
20221022T041503
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250220106
20221022T051509
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250220107
20221022T061503
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250220108
20221022T071509
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250220109
20221022T081503
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250220110
20221022T091509
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250220111
20221022T101502
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250220112
20221022T105503
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250220113
20221022T121503
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250220114
20221022T131509
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250220115
20221022T141503
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250220116
20221022T151509
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250220117
20221022T161503
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250220118
20221022T171509
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250220119
20221022T181503
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250220120
20221022T191503
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250220121
20221022T201503
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250220122
20221022T211503
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250220123
20221022T221509
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250230101
20221023T001503
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250230102
20221023T011503
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250230103
20221023T021509
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250230104
20221023T031503
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250230105
20221023T041509
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250230106
20221023T051503
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250230107
20221023T061509
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250230108
20221023T071503
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250230109
20221023T081509
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250230110
20221023T091503
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250230111
20221023T101509
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250230112
20221023T111503
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250230113
20221023T121509
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250230114
20221023T131003
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250230115
20221023T141503
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250230116
20221023T151503
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250230117
20221023T161508
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250230118
20221023T171503
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250230119
20221023T181509
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250230120
20221023T191503
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250230121
20221023T201503
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250230122
20221023T211510
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250230123
20221023T221503
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250230124
20221023T231509
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250240504
20221024T031503
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250240505
20221024T041508
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250240506
20221024T051503
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250240507
20221024T061509
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250240508
20221024T071503
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250240509
20221024T081509
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250240510
20221024T091503
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250240511
20221024T101509
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250240512
20221024T111503
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250240513
20221024T121509
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250240514
20221024T131003
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250240515
20221024T141503
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250240516
20221024T151508
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250240517
20221024T161503
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250240518
20221024T171509
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250240519
20221024T181503
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250240520
20221024T191503
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250240521
20221024T201503
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250240522
20221024T211509
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250240523
20221024T221503
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250240524
20221024T232003
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250250501
20221025T001503
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250250502
20221025T011503
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250250503
20221025T021510
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250250504
20221025T031503
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250250505
20221025T041509
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250250506
20221025T051503
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250250507
20221025T061510
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250250508
20221025T071503
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250250509
20221025T081509
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250250510
20221025T091503
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250250511
20221025T101508
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250250512
20221025T111503
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250250513
20221025T121508
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250250514
20221025T131003
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250250515
20221025T141503
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250250516
20221025T151503
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250250517
20221025T161509
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250250518
20221025T171503
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250250519
20221025T181509
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250250520
20221025T191502
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250250521
20221025T201503
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250250522
20221025T211509
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250250523
20221025T221503
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250250524
20221025T231509
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250260505
20221026T041503
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250260506
20221026T051509
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250260507
20221026T061503
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250260508
20221026T071509
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250260509
20221026T081503
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250260510
20221026T091508
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250260511
20221026T101503
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250260512
20221026T111508
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250260513
20221026T121503
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250260514
20221026T131508
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250260515
20221026T141503
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250260516
20221026T151509
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250260517
20221026T161503
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250260518
20221026T171508
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250260519
20221026T181503
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250260520
20221026T191509
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250260521
20221026T201502
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250260522
20221026T211503
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250260523
20221026T221509
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
250260524
20221026T231509
ISS off
Residual artificial line shift
V_LOS not released 		Degraded spatial resolution & polarimetric sensitivity
Spectral line shifted to the red due to etalon artefacts
V_LOS not released due to remaining artefacts
343220102
20230322T001408
Optical aberrations reisduals The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
343220103
20230322T002508
Optical aberrations reisduals The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
343220104
20230322T003608
Optical aberrations reisduals The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
343220105
20230322T004708
Optical aberrations reisduals The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
343220106
20230322T005808
Optical aberrations reisduals The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
343220107
20230322T010908
Optical aberrations reisduals The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
343220108
20230322T012008
Optical aberrations reisduals The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
343220109
20230322T013108
Optical aberrations reisduals The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
343220110
20230322T014208
Optical aberrations reisduals The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
343220111
20230322T015308
Optical aberrations reisduals The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
343220112
20230322T020408
Optical aberrations reisduals The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
343220113
20230322T021508
Optical aberrations reisduals The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
343220114
20230322T022608
Optical aberrations reisduals The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
343220115
20230322T023708
Optical aberrations reisduals The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
343220116
20230322T024808
Optical aberrations reisduals The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
343220117
20230322T025908
Optical aberrations reisduals The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
343220118
20230322T031008
Optical aberrations reisduals The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
343220119
20230322T032108
Optical aberrations reisduals The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
343220120
20230322T033208
Optical aberrations reisduals The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
343220121
20230322T034308
Optical aberrations reisduals The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
343220122
20230322T035408
Optical aberrations reisduals The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
343220123
20230322T040508
Optical aberrations reisduals The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
343220124
20230322T041608
Optical aberrations reisduals The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
343220125
20230322T042708
Optical aberrations reisduals The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
343280101
20230328T034509
PMP temperature not stable
Optical aberrations reisduals
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
343280102
20230328T044508
PMP temperature not stable
Optical aberrations reisduals
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
343280103
20230328T080009
PMP temperature not stable
Optical aberrations reisduals
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
343280104
20230328T090009
PMP temperature not stable
Optical aberrations reisduals
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
343280105
20230328T120009
PMP temperature not stable
Optical aberrations reisduals
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
343280106
20230328T130008
PMP temperature not stable
Optical aberrations reisduals
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
343280107
20230328T160009
PMP temperature not stable
Optical aberrations reisduals
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
343280108
20230328T170008
PMP temperature not stable
Optical aberrations reisduals
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
343280109
20230328T193009
PMP temperature not stable
Optical aberrations reisduals
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
343280110
20230328T203008
PMP temperature not stable
Optical aberrations reisduals
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
343290101
20230329T004509
PMP temperature not stable
Optical aberrations reisduals
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
343290102
20230329T040009
PMP temperature not stable
Optical aberrations reisduals
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
343290103
20230329T050008
PMP temperature not stable
Optical aberrations reisduals
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
343290104
20230329T060508
PMP temperature not stable
Optical aberrations reisduals
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
343290105
20230329T062008
PMP temperature not stable
Optical aberrations reisduals
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
343290106
20230329T064008
PMP temperature not stable
Optical aberrations reisduals
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
343290107
20230329T065508
PMP temperature not stable
Optical aberrations reisduals
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
343290701
20230329T114009
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290702
20230329T114109
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290703
20230329T114209
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290704
20230329T114309
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290705
20230329T114409
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290706
20230329T114509
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290707
20230329T114609
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290708
20230329T114709
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290709
20230329T114809
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290710
20230329T114909
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290711
20230329T115009
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290712
20230329T115109
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290713
20230329T115209
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290714
20230329T115309
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290715
20230329T115409
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290716
20230329T115509
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290717
20230329T115609
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290718
20230329T115709
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290719
20230329T115809
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290720
20230329T115909
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290721
20230329T120009
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290722
20230329T120109
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290723
20230329T120209
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290724
20230329T120309
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290725
20230329T120409
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290726
20230329T120509
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290727
20230329T120609
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290728
20230329T120709
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290729
20230329T120809
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290730
20230329T120909
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290731
20230329T121009
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290732
20230329T121109
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290733
20230329T121209
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290734
20230329T121309
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290735
20230329T121409
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290736
20230329T121509
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290737
20230329T121609
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290738
20230329T121709
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290739
20230329T121809
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290740
20230329T121909
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290741
20230329T122009
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290742
20230329T122109
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290743
20230329T122209
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290744
20230329T122309
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290745
20230329T122409
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290746
20230329T122509
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290747
20230329T122609
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290748
20230329T122709
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290749
20230329T122809
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290750
20230329T122909
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290751
20230329T123009
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290752
20230329T123109
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290753
20230329T123209
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290754
20230329T123309
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290755
20230329T123409
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290756
20230329T123509
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290757
20230329T123609
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290758
20230329T123709
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290759
20230329T123809
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290760
20230329T123909
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290761
20230329T124009
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290762
20230329T124109
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290763
20230329T124209
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290764
20230329T124309
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290765
20230329T124409
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290766
20230329T124509
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290767
20230329T124609
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290768
20230329T124709
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290769
20230329T124809
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290770
20230329T124909
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290771
20230329T125009
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290772
20230329T125109
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290773
20230329T125209
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290774
20230329T125309
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290775
20230329T125409
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290776
20230329T125509
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290777
20230329T125609
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290778
20230329T125709
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290779
20230329T125809
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290780
20230329T125909
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290781
20230329T130009
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290782
20230329T130109
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290783
20230329T130209
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290784
20230329T130309
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290785
20230329T130409
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290786
20230329T130509
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290787
20230329T130609
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290788
20230329T130709
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290789
20230329T130809
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290790
20230329T130909
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290791
20230329T131009
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290792
20230329T131109
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290793
20230329T131209
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290794
20230329T131309
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290795
20230329T131409
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290796
20230329T131509
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290797
20230329T131609
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290798
20230329T131709
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290799
20230329T131809
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290800
20230329T131909
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290801
20230329T132009
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290802
20230329T132109
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290803
20230329T132209
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290804
20230329T132309
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290805
20230329T132409
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290806
20230329T132509
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290807
20230329T132609
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290808
20230329T132709
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290809
20230329T132809
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290810
20230329T132909
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290811
20230329T133009
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290812
20230329T133109
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290813
20230329T133209
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290814
20230329T133309
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290815
20230329T133409
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290816
20230329T133509
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290817
20230329T133609
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290818
20230329T133709
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290819
20230329T133809
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290820
20230329T133909
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290821
20230329T134009
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290822
20230329T134109
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290823
20230329T134209
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290824
20230329T134309
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290825
20230329T134409
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290826
20230329T134509
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290827
20230329T134609
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290828
20230329T134709
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290829
20230329T134809
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290830
20230329T134909
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290831
20230329T135009
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290832
20230329T135109
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290833
20230329T135209
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290834
20230329T135309
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290835
20230329T135409
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290836
20230329T135509
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290837
20230329T135609
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290838
20230329T135709
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290839
20230329T135809
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290840
20230329T135909
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290841
20230329T140009
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290842
20230329T140109
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290843
20230329T140209
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290844
20230329T140309
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290845
20230329T140409
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290846
20230329T140509
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290847
20230329T140609
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290848
20230329T140709
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290849
20230329T140809
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290850
20230329T140909
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290851
20230329T141009
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290852
20230329T141109
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290853
20230329T141209
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290854
20230329T141309
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290855
20230329T141409
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290856
20230329T141509
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290857
20230329T141609
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290858
20230329T141709
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290859
20230329T141809
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290860
20230329T141909
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290861
20230329T142009
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290862
20230329T142109
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290863
20230329T142209
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290864
20230329T142309
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290865
20230329T142409
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290866
20230329T142509
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290867
20230329T142609
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290868
20230329T142709
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290869
20230329T142809
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290870
20230329T142909
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290871
20230329T143009
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290872
20230329T143109
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290873
20230329T143209
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290874
20230329T143309
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290875
20230329T143409
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290876
20230329T143509
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290877
20230329T143609
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290878
20230329T143709
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290879
20230329T143809
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290880
20230329T143909
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290881
20230329T144009
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290882
20230329T144109
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290883
20230329T144209
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290884
20230329T144309
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290885
20230329T144409
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290886
20230329T144509
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290887
20230329T144609
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290888
20230329T144709
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290889
20230329T144809
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290890
20230329T144909
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290891
20230329T145009
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290892
20230329T145109
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290893
20230329T145209
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290894
20230329T145309
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290895
20230329T145409
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290896
20230329T145509
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290897
20230329T145609
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290898
20230329T145709
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290899
20230329T145809
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290900
20230329T145909
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290901
20230329T150009
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290902
20230329T150109
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290903
20230329T150209
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290904
20230329T150309
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290905
20230329T150409
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290906
20230329T150509
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290907
20230329T150609
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290908
20230329T150709
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290909
20230329T150809
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290910
20230329T150909
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290911
20230329T151009
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290912
20230329T151109
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290913
20230329T151209
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290914
20230329T151309
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290915
20230329T151409
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290916
20230329T151509
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290917
20230329T151609
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290918
20230329T151709
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290919
20230329T151809
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290920
20230329T151909
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290921
20230329T152009
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290922
20230329T152109
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290923
20230329T152209
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290924
20230329T152309
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290925
20230329T152409
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290926
20230329T152509
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290927
20230329T152609
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290928
20230329T152709
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290929
20230329T152809
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290930
20230329T152909
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290931
20230329T153009
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290932
20230329T153109
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290933
20230329T153209
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290934
20230329T153309
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290935
20230329T153409
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290936
20230329T153509
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290937
20230329T153609
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290938
20230329T153709
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290939
20230329T153809
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
343290940
20230329T153909
PMP temperature not stable
4 Bits compression
 The temperature of the PMP was commanded wrongly and the it was floating at ~46 deg instead of 50.
The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
344010101
20230401T150009
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
344010102
20230401T160009
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
344040601
20230404T040809
4 Bits compression
Dust grain remnants in icnt
 The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
344040602
20230404T050809
4 Bits compression
Dust grain remnants in icnt
 The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
344040603
20230404T060809
4 Bits compression
Dust grain remnants in icnt
 The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
344040604
20230404T061809
4 Bits compression
Dust grain remnants in icnt
 The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
344040605
20230404T061949
4 Bits compression
Dust grain remnants in icnt
 The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
344040606
20230404T062129
4 Bits compression
Dust grain remnants in icnt
 The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
344040607
20230404T062309
4 Bits compression
Dust grain remnants in icnt
 The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
344040608
20230404T062449
4 Bits compression
Dust grain remnants in icnt
 The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
344040609
20230404T062629
4 Bits compression
Dust grain remnants in icnt
 The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
344040610
20230404T062809
4 Bits compression
Dust grain remnants in icnt
 The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
344040611
20230404T062949
4 Bits compression
Dust grain remnants in icnt
 The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
344040612
20230404T063129
4 Bits compression
Dust grain remnants in icnt
 The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
344040613
20230404T063309
4 Bits compression
Dust grain remnants in icnt
 The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
344040614
20230404T063449
4 Bits compression
Dust grain remnants in icnt
 The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
344040615
20230404T063629
4 Bits compression
Dust grain remnants in icnt
 The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
344040616
20230404T063809
4 Bits compression
Dust grain remnants in icnt
 The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
344040617
20230404T063949
4 Bits compression
Dust grain remnants in icnt
 The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
344040618
20230404T064129
4 Bits compression
Dust grain remnants in icnt
 The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
344040619
20230404T064309
4 Bits compression
Dust grain remnants in icnt
 The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
344040620
20230404T064449
4 Bits compression
Dust grain remnants in icnt
 The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
344040621
20230404T064629
4 Bits compression
Dust grain remnants in icnt
 The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
344040622
20230404T070809
4 Bits compression
Dust grain remnants in icnt
 The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
344040701
20230404T120009
4 Bits compression
Dust grain remnants in icnt
 The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
344040702
20230404T123009
4 Bits compression
Dust grain remnants in icnt
 The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
344040703
20230404T130009
4 Bits compression
Dust grain remnants in icnt
 The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
344040704
20230404T133009
4 Bits compression
Dust grain remnants in icnt
 The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
344040705
20230404T140009
4 Bits compression
Dust grain remnants in icnt
 The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
344040706
20230404T143009
4 Bits compression
Dust grain remnants in icnt
 The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
344040707
20230404T150009
4 Bits compression
Dust grain remnants in icnt
 The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
344040709
20230404T160009
4 Bits compression
Dust grain remnants in icnt
 The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
344040710
20230404T163009
4 Bits compression
Dust grain remnants in icnt
 The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
344040711
20230404T170009
4 Bits compression
Dust grain remnants in icnt
 The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
344040712
20230404T173009
4 Bits compression
Dust grain remnants in icnt
 The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
344040713
20230404T180009
4 Bits compression
Dust grain remnants in icnt
 The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
344040714
20230404T183009
4 Bits compression
Dust grain remnants in icnt
 The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
344040715
20230404T190009
4 Bits compression
Dust grain remnants in icnt
 The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
344040716
20230404T200009
4 Bits compression
Dust grain remnants in icnt
 The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
344050601
20230405T010009
4 Bits compression
Dust grain remnants in icnt
 The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
344050602
20230405T013009
4 Bits compression
Dust grain remnants in icnt
 The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
344050603
20230405T020009
4 Bits compression
Dust grain remnants in icnt
 The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
344050604
20230405T023009
4 Bits compression
Dust grain remnants in icnt
 The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
344050605
20230405T030009
4 Bits compression
Dust grain remnants in icnt
 The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
344050606
20230405T033009
4 Bits compression
Dust grain remnants in icnt
 The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
344050607
20230405T040009
4 Bits compression
Dust grain remnants in icnt
 The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
344050608
20230405T043009
4 Bits compression
Dust grain remnants in icnt
 The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
344050609
20230405T050009
4 Bits compression
Dust grain remnants in icnt
 The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
344050610
20230405T053009
4 Bits compression
Dust grain remnants in icnt
 The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
344050611
20230405T060009
4 Bits compression
Dust grain remnants in icnt
 The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
344050612
20230405T063009
4 Bits compression
Dust grain remnants in icnt
 The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
344050613
20230405T070009
4 Bits compression
Dust grain remnants in icnt
 The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
344050614
20230405T073009
4 Bits compression
Dust grain remnants in icnt
 The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
344050615
20230405T080009
4 Bits compression
Dust grain remnants in icnt
 The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
344070601
20230407T032009
4 Bits compression
Dust grain remnants in icnt
Flat field introduces gradient in icnt
 The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344070602
20230407T042009
4 Bits compression
Dust grain remnants in icnt
Flat field introduces gradient in icnt
 The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344070603
20230407T045010
4 Bits compression
Dust grain remnants in icnt
Flat field introduces gradient in icnt
 The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344070604
20230407T045150
4 Bits compression
Dust grain remnants in icnt
Flat field introduces gradient in icnt
 The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344070605
20230407T045330
4 Bits compression
Dust grain remnants in icnt
Flat field introduces gradient in icnt
 The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344070606
20230407T045510
4 Bits compression
Dust grain remnants in icnt
Flat field introduces gradient in icnt
 The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344070607
20230407T045650
4 Bits compression
Dust grain remnants in icnt
Flat field introduces gradient in icnt
 The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344070608
20230407T045830
4 Bits compression
Dust grain remnants in icnt
Flat field introduces gradient in icnt
 The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344070609
20230407T050010
4 Bits compression
Dust grain remnants in icnt
Flat field introduces gradient in icnt
 The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344070610
20230407T050150
4 Bits compression
Dust grain remnants in icnt
Flat field introduces gradient in icnt
 The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344070611
20230407T050330
4 Bits compression
Dust grain remnants in icnt
Flat field introduces gradient in icnt
 The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344070612
20230407T050510
4 Bits compression
Dust grain remnants in icnt
Flat field introduces gradient in icnt
 The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344070613
20230407T050650
4 Bits compression
Dust grain remnants in icnt
Flat field introduces gradient in icnt
 The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344070614
20230407T050830
4 Bits compression
Dust grain remnants in icnt
Flat field introduces gradient in icnt
 The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344070615
20230407T051010
4 Bits compression
Dust grain remnants in icnt
Flat field introduces gradient in icnt
 The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344070616
20230407T051150
4 Bits compression
Dust grain remnants in icnt
Flat field introduces gradient in icnt
 The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344070617
20230407T051330
4 Bits compression
Dust grain remnants in icnt
Flat field introduces gradient in icnt
 The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344070618
20230407T051510
4 Bits compression
Dust grain remnants in icnt
Flat field introduces gradient in icnt
 The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344070619
20230407T051650
4 Bits compression
Dust grain remnants in icnt
Flat field introduces gradient in icnt
 The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344070620
20230407T051830
4 Bits compression
Dust grain remnants in icnt
Flat field introduces gradient in icnt
 The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344070621
20230407T055009
4 Bits compression
Dust grain remnants in icnt
Flat field introduces gradient in icnt
 The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100501
20230410T033009
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100502
20230410T033109
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100503
20230410T033209
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100504
20230410T033309
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100505
20230410T033409
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100506
20230410T033509
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100507
20230410T033609
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100508
20230410T033709
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100509
20230410T033809
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100510
20230410T033909
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100511
20230410T034009
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100512
20230410T034109
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100513
20230410T034209
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100514
20230410T034309
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100515
20230410T034409
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100516
20230410T034509
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100517
20230410T034609
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100518
20230410T034709
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100519
20230410T034809
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100520
20230410T034909
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100521
20230410T035009
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100522
20230410T035109
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100523
20230410T035209
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100524
20230410T035309
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100525
20230410T035409
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100526
20230410T035509
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100527
20230410T035609
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100528
20230410T035709
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100529
20230410T035809
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100530
20230410T035909
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100531
20230410T040009
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100532
20230410T040109
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100533
20230410T040209
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100534
20230410T040309
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100535
20230410T040409
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100536
20230410T040509
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100537
20230410T040609
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100538
20230410T040709
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100539
20230410T040809
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100540
20230410T040909
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100541
20230410T041009
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100542
20230410T041109
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100543
20230410T041209
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100544
20230410T041309
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100545
20230410T041409
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100546
20230410T041509
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100547
20230410T041609
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100548
20230410T041709
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100549
20230410T041809
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100550
20230410T041909
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100551
20230410T042009
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100552
20230410T042109
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100553
20230410T042209
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100554
20230410T042309
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100555
20230410T042409
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100556
20230410T042509
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100557
20230410T042609
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100558
20230410T042709
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100559
20230410T042809
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100560
20230410T042909
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100561
20230410T043009
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100562
20230410T043109
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100563
20230410T043209
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100564
20230410T043309
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100565
20230410T043409
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100566
20230410T043509
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100567
20230410T043609
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100568
20230410T043709
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100569
20230410T043809
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100570
20230410T043909
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100571
20230410T044009
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100572
20230410T044109
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100573
20230410T044209
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100574
20230410T044309
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100575
20230410T044409
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100576
20230410T044509
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100577
20230410T044609
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100578
20230410T044709
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100579
20230410T044809
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100580
20230410T044909
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100581
20230410T045009
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100582
20230410T045109
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100583
20230410T045209
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100584
20230410T045309
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100585
20230410T045409
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100586
20230410T045509
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100587
20230410T045609
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100588
20230410T045709
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100589
20230410T045809
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100590
20230410T045909
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100591
20230410T050009
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100592
20230410T050109
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100593
20230410T050209
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100594
20230410T050309
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100595
20230410T050409
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100596
20230410T050509
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100597
20230410T050609
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100598
20230410T050709
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100599
20230410T050809
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100600
20230410T050909
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100601
20230410T051009
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100602
20230410T051109
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100603
20230410T051209
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100604
20230410T051309
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100605
20230410T051409
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100606
20230410T051509
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100607
20230410T051609
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100608
20230410T051709
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100609
20230410T051809
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100610
20230410T051909
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100611
20230410T052009
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100612
20230410T052109
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100613
20230410T052209
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100614
20230410T052309
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100615
20230410T052409
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100616
20230410T052509
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100617
20230410T052609
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100618
20230410T052709
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100619
20230410T052809
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100620
20230410T052909
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100621
20230410T053009
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100622
20230410T053109
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100623
20230410T053209
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100624
20230410T053309
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100625
20230410T053409
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100626
20230410T053509
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100627
20230410T053609
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100628
20230410T053709
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100629
20230410T053809
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100630
20230410T053909
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100631
20230410T054009
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100632
20230410T054109
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100633
20230410T054209
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100634
20230410T054309
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100635
20230410T054409
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100636
20230410T054509
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100637
20230410T054609
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100638
20230410T054709
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100639
20230410T054809
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100640
20230410T054909
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100641
20230410T055009
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100642
20230410T055109
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100643
20230410T055209
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100644
20230410T055309
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100645
20230410T055409
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100646
20230410T055509
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100647
20230410T055609
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100648
20230410T055709
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100649
20230410T055809
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100650
20230410T055909
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100651
20230410T060009
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100652
20230410T060109
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100653
20230410T060209
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100654
20230410T060309
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100655
20230410T060409
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100656
20230410T060509
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100657
20230410T060609
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100658
20230410T060709
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100659
20230410T060809
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100660
20230410T060909
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100661
20230410T061009
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100662
20230410T061109
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100663
20230410T061209
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100664
20230410T061309
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100665
20230410T061409
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100666
20230410T061509
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100667
20230410T061609
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100668
20230410T061709
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100669
20230410T061809
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100670
20230410T061909
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100671
20230410T062009
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100672
20230410T062109
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100673
20230410T062209
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100674
20230410T062309
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100675
20230410T062409
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100676
20230410T062509
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100677
20230410T062609
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100678
20230410T062709
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100679
20230410T062809
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100680
20230410T062909
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100681
20230410T063009
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100682
20230410T063109
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100683
20230410T063209
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100684
20230410T063309
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100685
20230410T063409
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100686
20230410T063509
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100687
20230410T063609
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100688
20230410T063709
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100689
20230410T063809
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100690
20230410T063909
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100691
20230410T064009
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100692
20230410T064109
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100693
20230410T064209
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100694
20230410T064309
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100695
20230410T064409
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100696
20230410T064509
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100697
20230410T064609
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100698
20230410T064709
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100699
20230410T064809
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100700
20230410T064909
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100701
20230410T065009
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100702
20230410T065109
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100703
20230410T065209
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100704
20230410T065309
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100705
20230410T065409
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100706
20230410T065509
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100707
20230410T065609
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100708
20230410T065709
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100709
20230410T065809
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100710
20230410T065909
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100711
20230410T070009
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100712
20230410T070109
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100713
20230410T070209
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100714
20230410T070309
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100715
20230410T070409
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100716
20230410T070509
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100717
20230410T070609
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100718
20230410T070709
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100719
20230410T070809
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100720
20230410T070909
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100721
20230410T071009
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100722
20230410T071109
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100723
20230410T071209
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100724
20230410T071309
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100725
20230410T071409
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100726
20230410T071509
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100727
20230410T071609
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100728
20230410T071709
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100729
20230410T071809
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100730
20230410T071909
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100731
20230410T072009
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100732
20230410T072109
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100733
20230410T072209
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100734
20230410T072309
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100735
20230410T072409
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100736
20230410T072509
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100737
20230410T072609
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100738
20230410T072709
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100739
20230410T072809
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100740
20230410T072909
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100741
20230410T073009
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100742
20230410T073109
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100743
20230410T073209
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100744
20230410T073309
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100745
20230410T073409
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100746
20230410T073509
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100747
20230410T073609
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100748
20230410T073709
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100749
20230410T073809
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100750
20230410T073909
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100751
20230410T074009
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100752
20230410T074109
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100753
20230410T074209
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100754
20230410T074309
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100755
20230410T074409
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100756
20230410T074509
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100757
20230410T074609
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100758
20230410T074709
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100759
20230410T074809
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100760
20230410T074909
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100761
20230410T075009
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100762
20230410T075109
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100763
20230410T075209
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100764
20230410T075309
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100765
20230410T075409
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100766
20230410T075509
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100767
20230410T075609
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100768
20230410T075709
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100769
20230410T075809
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100770
20230410T075909
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100771
20230410T080009
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100772
20230410T080109
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100773
20230410T080209
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100774
20230410T080309
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100775
20230410T080409
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100776
20230410T080509
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100777
20230410T080609
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100778
20230410T080709
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100779
20230410T080809
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100780
20230410T080909
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100781
20230410T081009
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100782
20230410T081109
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100783
20230410T081209
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100784
20230410T081309
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100785
20230410T081409
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100786
20230410T081509
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100787
20230410T081609
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100788
20230410T081709
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100789
20230410T081809
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100790
20230410T081909
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100791
20230410T082009
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100792
20230410T082109
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100793
20230410T082209
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100794
20230410T082309
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100795
20230410T082409
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100796
20230410T082509
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100797
20230410T082609
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100798
20230410T082709
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100799
20230410T082809
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100800
20230410T082909
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100801
20230410T083009
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100802
20230410T083109
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100803
20230410T083209
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100804
20230410T083309
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100805
20230410T083409
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100806
20230410T083509
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100807
20230410T083609
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100808
20230410T083709
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100809
20230410T083809
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100810
20230410T083909
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100811
20230410T084009
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100812
20230410T084109
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100813
20230410T084209
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100814
20230410T084309
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100815
20230410T084409
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100816
20230410T084509
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100817
20230410T084609
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100818
20230410T084709
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100819
20230410T084809
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100820
20230410T084909
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100821
20230410T085009
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100822
20230410T085109
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100823
20230410T085209
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100824
20230410T085309
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100825
20230410T085409
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100826
20230410T085509
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100827
20230410T085609
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100828
20230410T085709
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100829
20230410T085809
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100830
20230410T085909
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100831
20230410T090009
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100832
20230410T090109
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100833
20230410T090209
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100834
20230410T090309
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100835
20230410T090409
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100836
20230410T090509
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100837
20230410T090609
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100838
20230410T090709
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100839
20230410T090809
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100840
20230410T090909
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100841
20230410T091009
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100842
20230410T091109
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100843
20230410T091209
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100844
20230410T091309
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100845
20230410T091409
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100846
20230410T091509
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100847
20230410T091609
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100848
20230410T091709
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100849
20230410T091809
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100850
20230410T091909
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100851
20230410T092009
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100852
20230410T092109
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100853
20230410T092209
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100854
20230410T092309
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100855
20230410T092409
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100856
20230410T092509
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100857
20230410T092609
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100858
20230410T092709
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100859
20230410T092809
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100860
20230410T092909
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100901
20230410T203009
4 Bits compression
Flat field introduces gradient in icnt
 The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100902
20230410T213009
4 Bits compression
Flat field introduces gradient in icnt
 The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100903
20230410T213109
4 Bits compression
Flat field introduces gradient in icnt
 The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100904
20230410T213209
4 Bits compression
Flat field introduces gradient in icnt
 The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100905
20230410T213309
4 Bits compression
Flat field introduces gradient in icnt
 The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100906
20230410T213409
4 Bits compression
Flat field introduces gradient in icnt
 The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100907
20230410T213509
4 Bits compression
Flat field introduces gradient in icnt
 The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100908
20230410T213609
4 Bits compression
Flat field introduces gradient in icnt
 The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100909
20230410T213709
4 Bits compression
Flat field introduces gradient in icnt
 The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100910
20230410T213809
4 Bits compression
Flat field introduces gradient in icnt
 The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100911
20230410T213909
4 Bits compression
Flat field introduces gradient in icnt
 The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100912
20230410T214009
4 Bits compression
Flat field introduces gradient in icnt
 The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100913
20230410T214109
4 Bits compression
Flat field introduces gradient in icnt
 The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100914
20230410T214209
4 Bits compression
Flat field introduces gradient in icnt
 The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100915
20230410T214309
4 Bits compression
Flat field introduces gradient in icnt
 The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100916
20230410T214409
4 Bits compression
Flat field introduces gradient in icnt
 The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100917
20230410T214509
4 Bits compression
Flat field introduces gradient in icnt
 The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100918
20230410T214609
4 Bits compression
Flat field introduces gradient in icnt
 The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100919
20230410T214709
4 Bits compression
Flat field introduces gradient in icnt
 The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100920
20230410T214809
4 Bits compression
Flat field introduces gradient in icnt
 The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100921
20230410T214909
4 Bits compression
Flat field introduces gradient in icnt
 The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100922
20230410T215009
4 Bits compression
Flat field introduces gradient in icnt
 The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100923
20230410T215109
4 Bits compression
Flat field introduces gradient in icnt
 The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100924
20230410T215209
4 Bits compression
Flat field introduces gradient in icnt
 The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100925
20230410T215309
4 Bits compression
Flat field introduces gradient in icnt
 The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100926
20230410T215409
4 Bits compression
Flat field introduces gradient in icnt
 The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100927
20230410T215509
4 Bits compression
Flat field introduces gradient in icnt
 The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100928
20230410T215609
4 Bits compression
Flat field introduces gradient in icnt
 The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100929
20230410T215709
4 Bits compression
Flat field introduces gradient in icnt
 The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100930
20230410T215809
4 Bits compression
Flat field introduces gradient in icnt
 The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100931
20230410T215909
4 Bits compression
Flat field introduces gradient in icnt
 The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344100932
20230410T230009
4 Bits compression
Flat field introduces gradient in icnt
 The data was compressd to 4 Bits (instead of 6) when downloaded. This results in higher compression noise.
The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344110101
20230411T211509
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344110102
20230411T221509
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344110103
20230411T231509
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344110104
20230411T231649
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344110105
20230411T231829
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344110106
20230411T232009
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344110107
20230411T232149
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344110108
20230411T232329
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344110109
20230411T232509
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344110110
20230411T232649
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344110111
20230411T232829
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344110112
20230411T233009
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344110113
20230411T233149
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344110114
20230411T233329
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344110115
20230411T233509
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344110116
20230411T233649
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344110117
20230411T233829
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344110118
20230411T234009
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344110119
20230411T234149
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344110120
20230411T234329
Flat field introduces gradient in icnt The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344150601
20230415T023503
Dust grain remnants in icnt
Optical aberrations reisduals
Flat field introduces gradient in icnt
 Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344150602
20230415T033503
Dust grain remnants in icnt
Optical aberrations reisduals
Flat field introduces gradient in icnt
 Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344150603
20230415T043503
Dust grain remnants in icnt
Optical aberrations reisduals
Flat field introduces gradient in icnt
 Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344150604
20230415T043649
Dust grain remnants in icnt
Optical aberrations reisduals
Flat field introduces gradient in icnt
 Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344150605
20230415T043829
Dust grain remnants in icnt
Optical aberrations reisduals
Flat field introduces gradient in icnt
 Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344150606
20230415T044009
Dust grain remnants in icnt
Optical aberrations reisduals
Flat field introduces gradient in icnt
 Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344150607
20230415T044149
Dust grain remnants in icnt
Optical aberrations reisduals
Flat field introduces gradient in icnt
 Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344150608
20230415T044329
Dust grain remnants in icnt
Optical aberrations reisduals
Flat field introduces gradient in icnt
 Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344150609
20230415T044509
Dust grain remnants in icnt
Optical aberrations reisduals
Flat field introduces gradient in icnt
 Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344150610
20230415T044649
Dust grain remnants in icnt
Optical aberrations reisduals
Flat field introduces gradient in icnt
 Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344150611
20230415T044829
Dust grain remnants in icnt
Optical aberrations reisduals
Flat field introduces gradient in icnt
 Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344150612
20230415T045009
Dust grain remnants in icnt
Optical aberrations reisduals
Flat field introduces gradient in icnt
 Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344150613
20230415T045149
Dust grain remnants in icnt
Optical aberrations reisduals
Flat field introduces gradient in icnt
 Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344150614
20230415T045329
Dust grain remnants in icnt
Optical aberrations reisduals
Flat field introduces gradient in icnt
 Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344150615
20230415T045509
Dust grain remnants in icnt
Optical aberrations reisduals
Flat field introduces gradient in icnt
 Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344150616
20230415T045649
Dust grain remnants in icnt
Optical aberrations reisduals
Flat field introduces gradient in icnt
 Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344150617
20230415T045829
Dust grain remnants in icnt
Optical aberrations reisduals
Flat field introduces gradient in icnt
 Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344150618
20230415T050009
Dust grain remnants in icnt
Optical aberrations reisduals
Flat field introduces gradient in icnt
 Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344150619
20230415T050149
Dust grain remnants in icnt
Optical aberrations reisduals
Flat field introduces gradient in icnt
 Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344150620
20230415T050329
Dust grain remnants in icnt
Optical aberrations reisduals
Flat field introduces gradient in icnt
 Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The flat field used for this dataset was taken while off-pointing. A gradinet in the intensity continuum and LoS velocity is introduced.
344150201
20230415T174502
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
344150203
20230415T234502
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
344160202
20230416T080002
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
344160206
20230416T220003
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
344170202
20230417T080002
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
344170203
20230417T160002
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350080203
20231008T154503
Different reconstruction algorithm The datasets of this SOOP are reconstructed using different algorithm in each day. The quality of the reconstruction changes.
350080204
20231008T164506
Different reconstruction algorithm The datasets of this SOOP are reconstructed using different algorithm in each day. The quality of the reconstruction changes.
350090201
20231009T203003
Different reconstruction algorithm The datasets of this SOOP are reconstructed using different algorithm in each day. The quality of the reconstruction changes.
350090202
20231009T213005
Different reconstruction algorithm The datasets of this SOOP are reconstructed using different algorithm in each day. The quality of the reconstruction changes.
350120601
20231012T001503
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350120602
20231012T011503
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350120603
20231012T021503
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350120604
20231012T031503
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350120605
20231012T041503
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350120606
20231012T051503
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350120607
20231012T061503
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350120608
20231012T071502
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350120609
20231012T081503
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350120610
20231012T091503
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350120611
20231012T101503
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350120612
20231012T111503
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350120613
20231012T121503
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350120614
20231012T131503
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350120615
20231012T141503
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350120616
20231012T151503
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350120617
20231012T161503
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350120618
20231012T171503
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350120619
20231012T181503
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350120620
20231012T191503
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350120621
20231012T201503
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350120622
20231012T211503
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350120623
20231012T221503
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350120624
20231012T231503
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350130601
20231013T001503
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350130602
20231013T011503
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350130603
20231013T021503
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350130604
20231013T031503
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350130605
20231013T041503
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350130606
20231013T051503
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350130607
20231013T061503
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350130608
20231013T071503
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350130609
20231013T081503
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350130610
20231013T091503
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350130611
20231013T101503
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350130612
20231013T111503
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350130613
20231013T121503
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350130614
20231013T131503
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350130615
20231013T141503
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350130616
20231013T151503
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350130617
20231013T161503
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350130618
20231013T171503
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350130619
20231013T181503
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350130620
20231013T191503
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350130621
20231013T201503
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350130622
20231013T211503
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350130623
20231013T221503
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350130624
20231013T231503
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350140601
20231014T001503
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350140602
20231014T011503
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350140603
20231014T021503
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350140604
20231014T031503
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350140605
20231014T041503
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350140606
20231014T051503
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350140607
20231014T061503
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350140608
20231014T071503
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350140609
20231014T081503
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350140610
20231014T091503
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350140611
20231014T101503
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350140612
20231014T111503
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350140613
20231014T121503
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350140614
20231014T131503
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350140615
20231014T141503
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350140616
20231014T151503
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350140617
20231014T161503
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350140618
20231014T171503
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350140619
20231014T181503
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350140620
20231014T191502
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350140621
20231014T201502
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350140622
20231014T211503
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350140623
20231014T221503
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350140624
20231014T231503
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350150604
20231015T031503
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350150605
20231015T041503
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350150606
20231015T051503
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350150607
20231015T061503
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350150608
20231015T071503
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350150609
20231015T081503
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350150610
20231015T091503
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350150611
20231015T101503
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350150612
20231015T111503
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350150613
20231015T121503
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350150614
20231015T131502
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350150615
20231015T141503
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350150616
20231015T151503
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350150617
20231015T161503
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350150618
20231015T171503
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350150619
20231015T181503
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350150620
20231015T191503
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350150621
20231015T201503
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350150622
20231015T211503
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350150623
20231015T221503
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350150624
20231015T231503
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350160601
20231016T001503
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350160602
20231016T011503
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350160603
20231016T021503
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350160604
20231016T031503
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350160605
20231016T041502
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350160606
20231016T051503
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350160607
20231016T061503
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350160608
20231016T071502
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350160609
20231016T081503
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350160610
20231016T091503
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350160611
20231016T101502
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350160612
20231016T111502
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350160613
20231016T121503
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350160614
20231016T131503
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350160615
20231016T141503
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350160616
20231016T151503
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350160617
20231016T161503
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350160618
20231016T171503
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350160619
20231016T181503
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350160620
20231016T191503
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350160621
20231016T201503
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350160622
20231016T211503
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350160623
20231016T221503
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350160624
20231016T231502
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350170601
20231017T001503
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350170602
20231017T011503
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350170603
20231017T021503
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350170604
20231017T031502
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350170605
20231017T041503
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350170606
20231017T051503
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350170607
20231017T061503
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350170608
20231017T071503
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350170609
20231017T081503
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350170610
20231017T091503
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350170611
20231017T101503
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350170612
20231017T105503
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
350170701
20231017T123003
Strong optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution only partially removed the optical aberrations that are very well visible in the data.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350170702
20231017T125004
Strong optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution only partially removed the optical aberrations that are very well visible in the data.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350170703
20231017T131004
Strong optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution only partially removed the optical aberrations that are very well visible in the data.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350170704
20231017T133004
Strong optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution only partially removed the optical aberrations that are very well visible in the data.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350170705
20231017T135004
Strong optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution only partially removed the optical aberrations that are very well visible in the data.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350170706
20231017T141004
Strong optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution only partially removed the optical aberrations that are very well visible in the data.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350170707
20231017T143003
Strong optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution only partially removed the optical aberrations that are very well visible in the data.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350170708
20231017T144004
Strong optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution only partially removed the optical aberrations that are very well visible in the data.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350170709
20231017T145004
Strong optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution only partially removed the optical aberrations that are very well visible in the data.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350170710
20231017T150004
Strong optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution only partially removed the optical aberrations that are very well visible in the data.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350170711
20231017T151004
Strong optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution only partially removed the optical aberrations that are very well visible in the data.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350170712
20231017T152004
Strong optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution only partially removed the optical aberrations that are very well visible in the data.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350170713
20231017T153003
Strong optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution only partially removed the optical aberrations that are very well visible in the data.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350170714
20231017T153150
Strong optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution only partially removed the optical aberrations that are very well visible in the data.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350170715
20231017T153329
Strong optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution only partially removed the optical aberrations that are very well visible in the data.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350170716
20231017T153510
Strong optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution only partially removed the optical aberrations that are very well visible in the data.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350170717
20231017T153649
Strong optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution only partially removed the optical aberrations that are very well visible in the data.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350170718
20231017T153830
Strong optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution only partially removed the optical aberrations that are very well visible in the data.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350170719
20231017T154009
Strong optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution only partially removed the optical aberrations that are very well visible in the data.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350170720
20231017T154150
Strong optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution only partially removed the optical aberrations that are very well visible in the data.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350170721
20231017T154329
Strong optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution only partially removed the optical aberrations that are very well visible in the data.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350170722
20231017T154510
Strong optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution only partially removed the optical aberrations that are very well visible in the data.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350170723
20231017T154649
Strong optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution only partially removed the optical aberrations that are very well visible in the data.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350170724
20231017T154830
Strong optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution only partially removed the optical aberrations that are very well visible in the data.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350170725
20231017T155009
Strong optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution only partially removed the optical aberrations that are very well visible in the data.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350170726
20231017T160003
Strong optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution only partially removed the optical aberrations that are very well visible in the data.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350170727
20231017T161004
Strong optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution only partially removed the optical aberrations that are very well visible in the data.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350170728
20231017T162004
Strong optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution only partially removed the optical aberrations that are very well visible in the data.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350170729
20231017T163004
Strong optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution only partially removed the optical aberrations that are very well visible in the data.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350170730
20231017T164004
Strong optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution only partially removed the optical aberrations that are very well visible in the data.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350170731
20231017T165004
Strong optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution only partially removed the optical aberrations that are very well visible in the data.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350170732
20231017T170004
Strong optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution only partially removed the optical aberrations that are very well visible in the data.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350170733
20231017T171004
Strong optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution only partially removed the optical aberrations that are very well visible in the data.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350170734
20231017T172004
Strong optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution only partially removed the optical aberrations that are very well visible in the data.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350170735
20231017T173004
Strong optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution only partially removed the optical aberrations that are very well visible in the data.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350170736
20231017T174004
Strong optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution only partially removed the optical aberrations that are very well visible in the data.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350170737
20231017T175004
Strong optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution only partially removed the optical aberrations that are very well visible in the data.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350170738
20231017T180004
Strong optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution only partially removed the optical aberrations that are very well visible in the data.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350170739
20231017T181004
Strong optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution only partially removed the optical aberrations that are very well visible in the data.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350170740
20231017T182004
Strong optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution only partially removed the optical aberrations that are very well visible in the data.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350170741
20231017T183004
Strong optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution only partially removed the optical aberrations that are very well visible in the data.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350170742
20231017T184004
Strong optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution only partially removed the optical aberrations that are very well visible in the data.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350170743
20231017T185004
Strong optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution only partially removed the optical aberrations that are very well visible in the data.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350170744
20231017T190004
Strong optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution only partially removed the optical aberrations that are very well visible in the data.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350170745
20231017T191004
Strong optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution only partially removed the optical aberrations that are very well visible in the data.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350170746
20231017T192004
Strong optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution only partially removed the optical aberrations that are very well visible in the data.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350170747
20231017T193004
Strong optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution only partially removed the optical aberrations that are very well visible in the data.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350170748
20231017T194004
Strong optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution only partially removed the optical aberrations that are very well visible in the data.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350170749
20231017T195004
Strong optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution only partially removed the optical aberrations that are very well visible in the data.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350170750
20231017T200004
Strong optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution only partially removed the optical aberrations that are very well visible in the data.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350170751
20231017T201004
Strong optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution only partially removed the optical aberrations that are very well visible in the data.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350170752
20231017T202004
Strong optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution only partially removed the optical aberrations that are very well visible in the data.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350170753
20231017T203004
Strong optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution only partially removed the optical aberrations that are very well visible in the data.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350170622
20231017T211503
Higher noise than usual The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350170623
20231017T221503
Higher noise than usual The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350170624
20231017T231503
Higher noise than usual The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350180601
20231018T001503
Higher noise than usual The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350180602
20231018T011503
Higher noise than usual The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350180603
20231018T021503
Higher noise than usual The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350180604
20231018T031503
Higher noise than usual The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350180605
20231018T041503
Higher noise than usual The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350180606
20231018T051503
Higher noise than usual The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350180607
20231018T061503
Higher noise than usual The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350180608
20231018T071503
Higher noise than usual The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350180609
20231018T081503
Higher noise than usual The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350180610
20231018T091503
Higher noise than usual The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350180611
20231018T101503
Higher noise than usual The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350180612
20231018T111503
Higher noise than usual The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350180613
20231018T121503
Higher noise than usual The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350180614
20231018T131503
Higher noise than usual The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350180615
20231018T141502
Higher noise than usual The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350180616
20231018T151503
Higher noise than usual The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350180617
20231018T161503
Higher noise than usual The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350180618
20231018T171503
Higher noise than usual The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350180619
20231018T181503
Higher noise than usual The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350180620
20231018T191503
Higher noise than usual The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350180621
20231018T201503
Higher noise than usual The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350180622
20231018T211503
Higher noise than usual The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350180623
20231018T221503
Higher noise than usual The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350180624
20231018T231503
Higher noise than usual The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350190601
20231019T001503
Higher noise than usual The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350190602
20231019T001649
Higher noise than usual The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350190603
20231019T011504
Higher noise than usual The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350190604
20231019T011649
Higher noise than usual The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350190605
20231019T021503
Higher noise than usual The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350190606
20231019T021649
Higher noise than usual The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350190607
20231019T031503
Higher noise than usual The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350190608
20231019T031649
Higher noise than usual The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350190609
20231019T041503
Higher noise than usual The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350190610
20231019T041649
Higher noise than usual The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350190611
20231019T051503
Higher noise than usual The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350190612
20231019T051650
Higher noise than usual The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350190613
20231019T061503
Higher noise than usual The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350190614
20231019T061649
Higher noise than usual The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350190615
20231019T071503
Higher noise than usual The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350190616
20231019T071650
Higher noise than usual The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350190617
20231019T081503
Higher noise than usual The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350190618
20231019T081650
Higher noise than usual The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350190619
20231019T091503
Higher noise than usual The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350190620
20231019T091649
Higher noise than usual The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350190621
20231019T101503
Higher noise than usual The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350190622
20231019T101650
Higher noise than usual The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350190623
20231019T111503
Higher noise than usual The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350190624
20231019T111649
Higher noise than usual The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350190625
20231019T121503
Higher noise than usual The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350190626
20231019T121650
Higher noise than usual The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350190627
20231019T131503
Higher noise than usual The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350190628
20231019T131650
Higher noise than usual The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350190629
20231019T141503
Higher noise than usual The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350190630
20231019T141649
Higher noise than usual The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350190631
20231019T151503
Higher noise than usual The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350190632
20231019T151649
Higher noise than usual The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350190633
20231019T161503
Higher noise than usual The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350190634
20231019T161649
Higher noise than usual The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350190635
20231019T171503
Higher noise than usual The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350190636
20231019T171649
Higher noise than usual The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350190637
20231019T181503
Higher noise than usual The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350190638
20231019T181649
Higher noise than usual The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350190639
20231019T191503
Higher noise than usual The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350190640
20231019T191650
Higher noise than usual The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350190641
20231019T201503
Higher noise than usual The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350190642
20231019T201650
Higher noise than usual The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350190643
20231019T211503
Higher noise than usual The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350190644
20231019T211650
Higher noise than usual The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350190645
20231019T221503
Higher noise than usual The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350190646
20231019T221649
Higher noise than usual The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350190647
20231019T231503
Higher noise than usual The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350190648
20231019T231650
Higher noise than usual The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200601
20231020T053003
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200602
20231020T053110
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200603
20231020T053210
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200604
20231020T053310
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200605
20231020T053410
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200606
20231020T053510
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200607
20231020T053610
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200608
20231020T053710
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200609
20231020T053810
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200610
20231020T053910
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200611
20231020T054010
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200612
20231020T054110
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200613
20231020T054210
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200614
20231020T054310
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200615
20231020T054410
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200616
20231020T054510
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200617
20231020T054610
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200618
20231020T054710
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200619
20231020T054810
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200620
20231020T054910
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200621
20231020T055010
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200622
20231020T055110
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200623
20231020T055210
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200624
20231020T055310
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200625
20231020T055410
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200626
20231020T055510
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200627
20231020T055610
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200628
20231020T055710
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200629
20231020T055810
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200630
20231020T055910
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200631
20231020T060010
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200632
20231020T060110
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200633
20231020T060210
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200634
20231020T060310
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200635
20231020T060410
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200636
20231020T060510
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200637
20231020T060610
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200638
20231020T060710
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200639
20231020T060810
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200640
20231020T060910
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200641
20231020T061010
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200642
20231020T061110
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200643
20231020T061210
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200644
20231020T061310
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200645
20231020T061410
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200646
20231020T061510
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200647
20231020T061610
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200648
20231020T061710
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200649
20231020T061810
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200650
20231020T061910
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200651
20231020T062010
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200652
20231020T062110
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200653
20231020T062210
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200654
20231020T062310
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200655
20231020T062410
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200656
20231020T062510
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200657
20231020T062610
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200658
20231020T062710
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200659
20231020T062810
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200660
20231020T062910
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200661
20231020T063010
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200662
20231020T063110
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200663
20231020T063210
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200664
20231020T063310
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200665
20231020T063410
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200666
20231020T063510
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200667
20231020T063610
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200668
20231020T063710
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200669
20231020T063810
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200670
20231020T063910
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200671
20231020T064010
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200672
20231020T064110
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200673
20231020T064210
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200674
20231020T064310
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200675
20231020T064410
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200676
20231020T064510
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200677
20231020T064610
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200678
20231020T064710
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200679
20231020T064810
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200680
20231020T064910
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200681
20231020T065010
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200682
20231020T065110
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200683
20231020T065210
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200684
20231020T065310
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200685
20231020T065410
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200686
20231020T065510
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200687
20231020T065610
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200688
20231020T065710
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200689
20231020T065810
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200690
20231020T065910
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200691
20231020T070010
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200692
20231020T070110
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200693
20231020T070210
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200694
20231020T070310
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200695
20231020T070410
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200696
20231020T070510
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200697
20231020T070610
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200698
20231020T070710
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200699
20231020T070810
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200700
20231020T070910
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200701
20231020T071010
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200702
20231020T071110
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200703
20231020T071210
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200704
20231020T071310
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200705
20231020T071410
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200706
20231020T071510
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200707
20231020T071610
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200708
20231020T071709
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200709
20231020T071809
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200710
20231020T071909
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200711
20231020T072009
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200712
20231020T072109
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200713
20231020T072209
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200714
20231020T072309
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200715
20231020T072409
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200716
20231020T072509
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200717
20231020T072609
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200718
20231020T072709
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200719
20231020T072809
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200720
20231020T072909
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200721
20231020T073009
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200722
20231020T073109
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200723
20231020T073209
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200724
20231020T073309
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200725
20231020T073409
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200726
20231020T073509
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200727
20231020T073609
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200728
20231020T073709
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200729
20231020T073809
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200730
20231020T073909
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200731
20231020T074009
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200732
20231020T074109
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200733
20231020T074209
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200734
20231020T074309
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200735
20231020T074409
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200736
20231020T074509
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200737
20231020T074609
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200738
20231020T074709
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200739
20231020T074809
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200740
20231020T074909
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200741
20231020T075009
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200742
20231020T075109
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200743
20231020T075209
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200744
20231020T075309
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200745
20231020T075409
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200746
20231020T075509
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200747
20231020T075609
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200748
20231020T075709
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200749
20231020T075809
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200750
20231020T075909
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200751
20231020T080009
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200752
20231020T080109
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200753
20231020T080209
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200754
20231020T080309
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200755
20231020T080409
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200756
20231020T080509
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200757
20231020T080609
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200758
20231020T080709
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200759
20231020T080809
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200760
20231020T080909
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200761
20231020T081009
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200762
20231020T081109
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200763
20231020T081209
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200764
20231020T081309
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200765
20231020T081409
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200766
20231020T081509
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200767
20231020T081609
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200768
20231020T081709
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200769
20231020T081809
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200770
20231020T081909
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200771
20231020T082009
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200772
20231020T082109
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200773
20231020T082209
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200774
20231020T082309
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200775
20231020T082409
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200776
20231020T082509
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200777
20231020T082609
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200778
20231020T082709
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200779
20231020T082809
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200780
20231020T082909
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200781
20231020T083009
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200782
20231020T083109
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200783
20231020T083209
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200784
20231020T083309
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200785
20231020T083409
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200786
20231020T083509
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200787
20231020T083609
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200788
20231020T083709
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200789
20231020T083809
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200790
20231020T083909
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200791
20231020T084009
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200792
20231020T084109
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200793
20231020T084209
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200794
20231020T084309
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200795
20231020T084409
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200796
20231020T084509
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200797
20231020T084609
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200798
20231020T084709
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200799
20231020T084809
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200800
20231020T084909
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200801
20231020T085009
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200802
20231020T085109
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200803
20231020T085209
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200804
20231020T085309
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200805
20231020T085409
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200806
20231020T085509
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200807
20231020T085609
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200808
20231020T085709
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200809
20231020T085809
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200810
20231020T085909
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200811
20231020T090009
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200812
20231020T090109
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200813
20231020T090209
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200814
20231020T090309
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200815
20231020T090409
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200816
20231020T090509
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200817
20231020T090609
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200818
20231020T090709
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200819
20231020T090809
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200820
20231020T090909
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200821
20231020T091009
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200822
20231020T091109
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200823
20231020T091209
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200824
20231020T091309
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200825
20231020T091409
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200826
20231020T091509
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200827
20231020T091609
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200828
20231020T091709
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200829
20231020T091809
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200830
20231020T091909
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200831
20231020T092009
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200832
20231020T092109
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200833
20231020T092209
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200834
20231020T092309
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200835
20231020T092409
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200836
20231020T092509
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200837
20231020T092609
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200838
20231020T092709
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200839
20231020T092809
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200840
20231020T092909
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200841
20231020T093009
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200842
20231020T093109
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200843
20231020T093209
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200844
20231020T093309
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200845
20231020T093409
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200846
20231020T093509
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200847
20231020T093609
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200848
20231020T093709
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200849
20231020T093809
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200850
20231020T093909
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200851
20231020T094009
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200852
20231020T094109
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200853
20231020T094209
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200854
20231020T094309
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200855
20231020T094409
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200856
20231020T094509
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200857
20231020T094609
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200858
20231020T094709
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200859
20231020T094809
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200860
20231020T094909
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200861
20231020T095009
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200862
20231020T095109
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200863
20231020T095209
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200864
20231020T095309
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200865
20231020T095409
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200866
20231020T095509
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200867
20231020T095609
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200868
20231020T095709
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200869
20231020T095809
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200870
20231020T095909
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200871
20231020T100009
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200872
20231020T100109
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200873
20231020T100209
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200874
20231020T100309
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200875
20231020T100409
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200876
20231020T100509
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200877
20231020T100609
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200878
20231020T100709
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200879
20231020T100809
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200880
20231020T100909
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200881
20231020T101009
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200882
20231020T101109
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200883
20231020T101209
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200884
20231020T101309
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200885
20231020T101409
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200886
20231020T101509
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200887
20231020T101609
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200888
20231020T101709
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200889
20231020T101809
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200890
20231020T101909
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200891
20231020T102009
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200892
20231020T102109
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200893
20231020T102209
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200894
20231020T102309
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200895
20231020T102409
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200896
20231020T102509
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200897
20231020T102609
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200898
20231020T102709
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200899
20231020T102809
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200900
20231020T102909
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200901
20231020T103009
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200902
20231020T103109
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200903
20231020T103209
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200904
20231020T103309
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200905
20231020T103409
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200906
20231020T103509
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200907
20231020T103609
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200908
20231020T103709
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200909
20231020T103809
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200910
20231020T103909
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200911
20231020T104009
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200912
20231020T104109
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200913
20231020T104209
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200914
20231020T104309
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200915
20231020T104409
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200916
20231020T104509
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200917
20231020T104609
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200918
20231020T104709
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200919
20231020T104809
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200920
20231020T104909
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200921
20231020T105009
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200922
20231020T105109
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200923
20231020T105209
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200924
20231020T105309
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200925
20231020T105409
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200926
20231020T105509
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200927
20231020T105609
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200928
20231020T105709
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200929
20231020T105809
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200930
20231020T105909
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200931
20231020T110009
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200932
20231020T110109
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200933
20231020T110209
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200934
20231020T110309
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200935
20231020T110409
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200936
20231020T110509
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200937
20231020T110609
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200938
20231020T110709
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200939
20231020T110809
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200940
20231020T110909
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200941
20231020T111009
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200942
20231020T111109
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200943
20231020T111209
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200944
20231020T111309
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200945
20231020T111409
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200946
20231020T111509
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200947
20231020T111609
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200948
20231020T111709
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200949
20231020T111809
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200950
20231020T111909
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200951
20231020T112009
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200952
20231020T112109
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200953
20231020T112209
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200954
20231020T112309
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200955
20231020T112409
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200956
20231020T112509
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200957
20231020T112609
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200958
20231020T112709
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200959
20231020T112809
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200960
20231020T112909
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200501
20231020T133003
Strong optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution only partially removed the optical aberrations that are very well visible in the data.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200502
20231020T173003
Strong optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution only partially removed the optical aberrations that are very well visible in the data.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350200503
20231020T213002
Strong optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution only partially removed the optical aberrations that are very well visible in the data.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350240101
20231024T114503
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350240102
20231024T134503
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350250101
20231025T090003
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350250102
20231025T110003
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350260101
20231026T090003
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350260102
20231026T110003
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
370270101
20231027T100202
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
370270102
20231027T101202
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
370270103
20231027T102203
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
370270104
20231027T103203
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
370270105
20231027T104203
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
370270106
20231027T105203
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
370270107
20231027T110203
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
370270108
20231027T111203
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
370270109
20231027T112203
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
370270110
20231027T113203
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
370270111
20231027T114203
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
370270112
20231027T115203
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
370270113
20231027T120202
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
370270114
20231027T121202
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
370270115
20231027T122202
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
370270116
20231027T123202
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
370270117
20231027T124202
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
370270118
20231027T125203
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
370270119
20231027T130203
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
370270120
20231027T131202
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
370270121
20231027T132202
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
370270122
20231027T133202
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
370270123
20231027T134202
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
370270124
20231027T135203
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
370270125
20231027T140202
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350280601
20231028T004503
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350280602
20231028T010003
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350280603
20231028T011503
Optical aberrations reisduals
Higher noise than usual
 The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350280701
20231028T070003
Dust grain remnants in icnt
Optical aberrations reisduals
Higher noise than usual
 Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350280702
20231028T070603
Dust grain remnants in icnt
Optical aberrations reisduals
Higher noise than usual
 Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350280703
20231028T071203
Dust grain remnants in icnt
Optical aberrations reisduals
Higher noise than usual
 Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350280704
20231028T071803
Dust grain remnants in icnt
Optical aberrations reisduals
Higher noise than usual
 Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350280705
20231028T072403
Dust grain remnants in icnt
Optical aberrations reisduals
Higher noise than usual
 Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350280706
20231028T073003
Dust grain remnants in icnt
Optical aberrations reisduals
Higher noise than usual
 Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350280707
20231028T073603
Dust grain remnants in icnt
Optical aberrations reisduals
Higher noise than usual
 Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350280708
20231028T074203
Dust grain remnants in icnt
Optical aberrations reisduals
Higher noise than usual
 Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350280801
20231028T114503
Dust grain remnants in icnt
Optical aberrations reisduals
Higher noise than usual
 Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350280802
20231028T121503
Dust grain remnants in icnt
Optical aberrations reisduals
Higher noise than usual
 Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350280803
20231028T124503
Dust grain remnants in icnt
Optical aberrations reisduals
Higher noise than usual
 Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350280804
20231028T131503
Dust grain remnants in icnt
Optical aberrations reisduals
Higher noise than usual
 Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350280805
20231028T134503
Dust grain remnants in icnt
Optical aberrations reisduals
Higher noise than usual
 Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350280806
20231028T141503
Dust grain remnants in icnt
Optical aberrations reisduals
Higher noise than usual
 Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350280807
20231028T144503
Dust grain remnants in icnt
Optical aberrations reisduals
Higher noise than usual
 Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350280808
20231028T151503
Dust grain remnants in icnt
Optical aberrations reisduals
Higher noise than usual
 Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350280809
20231028T154503
Dust grain remnants in icnt
Optical aberrations reisduals
Higher noise than usual
 Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350280810
20231028T161503
Dust grain remnants in icnt
Optical aberrations reisduals
Higher noise than usual
 Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350280811
20231028T164503
Dust grain remnants in icnt
Optical aberrations reisduals
Higher noise than usual
 Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350280812
20231028T171503
Dust grain remnants in icnt
Optical aberrations reisduals
Higher noise than usual
 Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350280813
20231028T174503
Dust grain remnants in icnt
Optical aberrations reisduals
Higher noise than usual
 Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350280814
20231028T181503
Dust grain remnants in icnt
Optical aberrations reisduals
Higher noise than usual
 Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350280815
20231028T184503
Dust grain remnants in icnt
Optical aberrations reisduals
Higher noise than usual
 Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350280604
20231028T220503
Dust grain remnants in icnt
Optical aberrations reisduals
Higher noise than usual
 Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350280605
20231028T222003
Dust grain remnants in icnt
Optical aberrations reisduals
Higher noise than usual
 Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350280606
20231028T223503
Dust grain remnants in icnt
Optical aberrations reisduals
Higher noise than usual
 Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350290701
20231029T070003
Dust grain remnants in icnt
Optical aberrations reisduals
Higher noise than usual
 Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350290702
20231029T070209
Dust grain remnants in icnt
Optical aberrations reisduals
Higher noise than usual
 Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350290703
20231029T070409
Dust grain remnants in icnt
Optical aberrations reisduals
Higher noise than usual
 Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350290704
20231029T070609
Dust grain remnants in icnt
Optical aberrations reisduals
Higher noise than usual
 Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350290705
20231029T070809
Dust grain remnants in icnt
Optical aberrations reisduals
Higher noise than usual
 Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350290706
20231029T071009
Dust grain remnants in icnt
Optical aberrations reisduals
Higher noise than usual
 Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350290707
20231029T071209
Dust grain remnants in icnt
Optical aberrations reisduals
Higher noise than usual
 Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350290708
20231029T071409
Dust grain remnants in icnt
Optical aberrations reisduals
Higher noise than usual
 Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350290709
20231029T071609
Dust grain remnants in icnt
Optical aberrations reisduals
Higher noise than usual
 Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350290710
20231029T071809
Dust grain remnants in icnt
Optical aberrations reisduals
Higher noise than usual
 Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350290601
20231029T221107
Dust grain remnants in icnt
Optical aberrations reisduals
Higher noise than usual
 Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350290602
20231029T222608
Dust grain remnants in icnt
Optical aberrations reisduals
Higher noise than usual
 Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350290603
20231029T224108
Dust grain remnants in icnt
Optical aberrations reisduals
Higher noise than usual
 Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350300601
20231030T220607
Dust grain remnants in icnt
Optical aberrations reisduals
Higher noise than usual
 Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350300602
20231030T222108
Dust grain remnants in icnt
Optical aberrations reisduals
Higher noise than usual
 Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350300603
20231030T223608
Dust grain remnants in icnt
Optical aberrations reisduals
Higher noise than usual
 Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350310601
20231031T110107
Dust grain remnants in icnt
Strong optical aberrations reisduals
Higher noise than usual
 Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The PSF deconvolution only partially removed the optical aberrations that are very well visible in the data.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350310602
20231031T112108
Dust grain remnants in icnt
Strong optical aberrations reisduals
Higher noise than usual
 Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The PSF deconvolution only partially removed the optical aberrations that are very well visible in the data.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350310603
20231031T114108
Dust grain remnants in icnt
Strong optical aberrations reisduals
Higher noise than usual
 Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The PSF deconvolution only partially removed the optical aberrations that are very well visible in the data.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350310604
20231031T120108
Dust grain remnants in icnt
Strong optical aberrations reisduals
Higher noise than usual
 Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The PSF deconvolution only partially removed the optical aberrations that are very well visible in the data.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350310605
20231031T122107
Dust grain remnants in icnt
Strong optical aberrations reisduals
Higher noise than usual
 Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The PSF deconvolution only partially removed the optical aberrations that are very well visible in the data.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350310606
20231031T122608
Dust grain remnants in icnt
Strong optical aberrations reisduals
Higher noise than usual
 Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The PSF deconvolution only partially removed the optical aberrations that are very well visible in the data.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350310607
20231031T123108
Dust grain remnants in icnt
Strong optical aberrations reisduals
Higher noise than usual
 Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The PSF deconvolution only partially removed the optical aberrations that are very well visible in the data.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350310608
20231031T123608
Dust grain remnants in icnt
Strong optical aberrations reisduals
Higher noise than usual
 Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The PSF deconvolution only partially removed the optical aberrations that are very well visible in the data.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350310609
20231031T124108
Dust grain remnants in icnt
Strong optical aberrations reisduals
Higher noise than usual
 Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The PSF deconvolution only partially removed the optical aberrations that are very well visible in the data.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350310610
20231031T124608
Dust grain remnants in icnt
Strong optical aberrations reisduals
Higher noise than usual
 Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The PSF deconvolution only partially removed the optical aberrations that are very well visible in the data.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350310611
20231031T125108
Dust grain remnants in icnt
Strong optical aberrations reisduals
Higher noise than usual
 Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The PSF deconvolution only partially removed the optical aberrations that are very well visible in the data.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350310612
20231031T125608
Dust grain remnants in icnt
Strong optical aberrations reisduals
Higher noise than usual
 Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The PSF deconvolution only partially removed the optical aberrations that are very well visible in the data.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350310613
20231031T130108
Dust grain remnants in icnt
Strong optical aberrations reisduals
Higher noise than usual
 Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The PSF deconvolution only partially removed the optical aberrations that are very well visible in the data.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350310614
20231031T130608
Dust grain remnants in icnt
Strong optical aberrations reisduals
Higher noise than usual
 Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The PSF deconvolution only partially removed the optical aberrations that are very well visible in the data.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350310615
20231031T131108
Dust grain remnants in icnt
Strong optical aberrations reisduals
Higher noise than usual
 Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The PSF deconvolution only partially removed the optical aberrations that are very well visible in the data.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350310616
20231031T133107
Dust grain remnants in icnt
Strong optical aberrations reisduals
Higher noise than usual
 Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The PSF deconvolution only partially removed the optical aberrations that are very well visible in the data.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350310617
20231031T135108
Dust grain remnants in icnt
Strong optical aberrations reisduals
Higher noise than usual
 Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The PSF deconvolution only partially removed the optical aberrations that are very well visible in the data.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
350310618
20231031T141108
Dust grain remnants in icnt
Strong optical aberrations reisduals
Higher noise than usual
 Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The PSF deconvolution only partially removed the optical aberrations that are very well visible in the data.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
351010601
20231101T005607
Dust grain remnants in icnt
Optical aberrations reisduals
Higher noise than usual
 Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
351010602
20231101T011108
Dust grain remnants in icnt
Optical aberrations reisduals
Higher noise than usual
 Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
351010603
20231101T012608
Dust grain remnants in icnt
Optical aberrations reisduals
Higher noise than usual
 Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
443190203
20240319T210209

Optical aberrations reisduals
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
443190201
20240319T200210

Optical aberrations reisduals
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
443190206
20240319T223209

Optical aberrations reisduals
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
443190205
20240319T220209

Optical aberrations reisduals
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
443190202
20240319T203209

Optical aberrations reisduals
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
443190207
20240319T230209

Optical aberrations reisduals
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
443190208
20240319T233209

Optical aberrations reisduals
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
443190204
20240319T213209

Optical aberrations reisduals
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
443200301
20240320T060809
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
443200303
20240320T143509
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
443200304
20240320T184009
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
443200302
20240320T101309
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
443200305
20240320T224509
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
443210304
20240321T193509
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
443210302
20240321T100009
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
443210301
20240321T042009
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
443210303
20240321T153009
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
443210305
20240321T230509
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
443220301
20240322T034509
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
443220302
20240322T104509
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
443220103
20240322T214708
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
443220102
20240322T214108
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
443220101
20240322T213509
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
443220105
20240322T215908
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
443220104
20240322T215308
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
443220106
20240322T220508
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
443220107
20240322T221108
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
443220108
20240322T221708
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
443220110
20240322T222908
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
443220109
20240322T222308
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
443230602
20240323T115509
Dust grain remnants in icnt
Optical aberrations reisduals
ISS unstable 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The ISS could not properly correlate during the observation causing artifacts and higer noise.
443230603
20240323T183009
Dust grain remnants in icnt
Optical aberrations reisduals
ISS unstable 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The ISS could not properly correlate during the observation causing artifacts and higer noise.
443230601
20240323T050009
Dust grain remnants in icnt
Optical aberrations reisduals
ISS unstable 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The ISS could not properly correlate during the observation causing artifacts and higer noise.
443230201
20240323T223009
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
443230203
20240323T233008
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
443230202
20240323T230008
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
443240202
20240324T003009
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
443240204
20240324T013008
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
443240201
20240324T000010
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
443240205
20240324T020008
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
443240203
20240324T010008
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
443310108
20240331T151738
Dust grain remnants in icnt
Last data ISS off 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The ISS was off during the acquisition of the last dataset of the SOOP
443310110
20240331T154509
Dust grain remnants in icnt
Last data ISS off 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The ISS was off during the acquisition of the last dataset of the SOOP
443310101
20240331T150009
Dust grain remnants in icnt
Last data ISS off 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The ISS was off during the acquisition of the last dataset of the SOOP
443310107
20240331T151508
Dust grain remnants in icnt
Last data ISS off 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The ISS was off during the acquisition of the last dataset of the SOOP
443310109
20240331T152008
Dust grain remnants in icnt
Last data ISS off 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The ISS was off during the acquisition of the last dataset of the SOOP
443310103
20240331T150508
Dust grain remnants in icnt
Last data ISS off 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The ISS was off during the acquisition of the last dataset of the SOOP
443310102
20240331T150238
Dust grain remnants in icnt
Last data ISS off 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The ISS was off during the acquisition of the last dataset of the SOOP
443310106
20240331T151238
Dust grain remnants in icnt
Last data ISS off 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The ISS was off during the acquisition of the last dataset of the SOOP
443310105
20240331T151008
Dust grain remnants in icnt
Last data ISS off 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The ISS was off during the acquisition of the last dataset of the SOOP
443310104
20240331T150738
Dust grain remnants in icnt
Last data ISS off 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The ISS was off during the acquisition of the last dataset of the SOOP
444010101
20240401T150009
Dust grain remnants in icnt
Last data ISS off 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The ISS was off during the acquisition of the last dataset of the SOOP
444010102
20240401T154509
Dust grain remnants in icnt
Last data ISS off 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The ISS was off during the acquisition of the last dataset of the SOOP
444020208
20240402T233009
ISS unstable
Optical aberrations reisduals
Dust grain remnants in icnt
Higher noise than usual 		The ISS could not properly correlate during the observation causing artifacts and higer noise.
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444020204
20240402T213009
ISS unstable
Optical aberrations reisduals
Dust grain remnants in icnt
Higher noise than usual 		The ISS could not properly correlate during the observation causing artifacts and higer noise.
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444020205
20240402T220009
ISS unstable
Optical aberrations reisduals
Dust grain remnants in icnt
Higher noise than usual 		The ISS could not properly correlate during the observation causing artifacts and higer noise.
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444020203
20240402T210009
ISS unstable
Optical aberrations reisduals
Dust grain remnants in icnt
Higher noise than usual 		The ISS could not properly correlate during the observation causing artifacts and higer noise.
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444020202
20240402T203009
ISS unstable
Optical aberrations reisduals
Dust grain remnants in icnt
Higher noise than usual 		The ISS could not properly correlate during the observation causing artifacts and higer noise.
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444020207
20240402T230009
ISS unstable
Optical aberrations reisduals
Dust grain remnants in icnt
Higher noise than usual 		The ISS could not properly correlate during the observation causing artifacts and higer noise.
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444020206
20240402T223009
ISS unstable
Optical aberrations reisduals
Dust grain remnants in icnt
Higher noise than usual 		The ISS could not properly correlate during the observation causing artifacts and higer noise.
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444020201
20240402T200003
ISS unstable
Optical aberrations reisduals
Dust grain remnants in icnt
Higher noise than usual 		The ISS could not properly correlate during the observation causing artifacts and higer noise.
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030701
20240403T200003
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030707
20240403T203007
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030711
20240403T205008
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030708
20240403T203507
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030706
20240403T202507
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030704
20240403T201507
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030714
20240403T210507
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030703
20240403T201007
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030713
20240403T210007
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030710
20240403T204507
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030705
20240403T202007
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030715
20240403T211503
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030717
20240403T211710
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030702
20240403T200507
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030709
20240403T204007
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030712
20240403T205507
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030716
20240403T211610
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030719
20240403T211909
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030718
20240403T211810
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030720
20240403T212010
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030721
20240403T212109
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030722
20240403T212210
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030723
20240403T212310
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030725
20240403T212510
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030724
20240403T212409
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030727
20240403T212709
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030726
20240403T212609
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030729
20240403T212909
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030730
20240403T213009
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030731
20240403T213110
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030732
20240403T213210
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030733
20240403T213310
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030735
20240403T213510
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030734
20240403T213410
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030728
20240403T212809
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030736
20240403T213609
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030737
20240403T213710
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030738
20240403T213809
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030741
20240403T214110
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030739
20240403T213909
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030740
20240403T214009
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030742
20240403T214210
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030746
20240403T214610
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030757
20240403T215710
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030748
20240403T214809
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030745
20240403T214510
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030747
20240403T214710
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030743
20240403T214309
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030753
20240403T215310
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030751
20240403T215109
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030749
20240403T214909
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030754
20240403T215410
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030744
20240403T214410
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030750
20240403T215010
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030755
20240403T215509
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030756
20240403T215609
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030758
20240403T215809
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030760
20240403T220009
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030759
20240403T215910
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030762
20240403T220209
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030752
20240403T215209
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030761
20240403T220110
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030766
20240403T220610
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030764
20240403T220409
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030763
20240403T220310
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030765
20240403T220509
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030768
20240403T220810
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030769
20240403T220909
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030767
20240403T220710
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030770
20240403T221009
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030773
20240403T221310
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030774
20240403T221410
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030771
20240403T221109
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030772
20240403T221210
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030777
20240403T221710
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030775
20240403T221510
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030776
20240403T221609
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030779
20240403T221909
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030778
20240403T221809
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030780
20240403T222010
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030781
20240403T222109
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030782
20240403T222210
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030787
20240403T222709
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030784
20240403T222409
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030783
20240403T222309
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030785
20240403T222509
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030792
20240403T223209
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030788
20240403T222809
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030794
20240403T223409
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030793
20240403T223309
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030786
20240403T222609
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030796
20240403T223609
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030790
20240403T223009
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030795
20240403T223509
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030798
20240403T223809
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030800
20240403T224009
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030789
20240403T222910
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030803
20240403T224309
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030797
20240403T223709
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030799
20240403T223909
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030791
20240403T223109
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030804
20240403T224409
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030802
20240403T224209
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030806
20240403T224609
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030801
20240403T224109
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030805
20240403T224509
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030807
20240403T224709
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030808
20240403T224809
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030809
20240403T224909
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030811
20240403T225109
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030814
20240403T225409
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030810
20240403T225009
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030812
20240403T225209
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030813
20240403T225309
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030817
20240403T225709
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030815
20240403T225509
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030818
20240403T225809
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030816
20240403T225609
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030819
20240403T225909
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030820
20240403T230009
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030821
20240403T230109
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030824
20240403T230409
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030828
20240403T230809
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030822
20240403T230209
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030829
20240403T230909
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030826
20240403T230609
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030823
20240403T230309
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030830
20240403T231009
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030825
20240403T230509
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030827
20240403T230709
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030831
20240403T231109
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030835
20240403T232007
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030834
20240403T231409
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030833
20240403T231309
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030836
20240403T232507
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030837
20240403T233103
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030839
20240403T234107
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030840
20240403T234607
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030842
20240403T235607
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030841
20240403T235107
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030838
20240403T233607
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030844
20240404T000607
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030843
20240404T000107
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030845
20240404T001107
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030846
20240404T001607
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030847
20240404T002107
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444030848
20240404T002607
Start ISS off
Multiple accumulation
Optical aberrations reisduals
Higher noise than usual 		The ISS was off during the acquisition of the first 14 datasets of the SOOP
The accumulation scheme (and consequently the noise) changes through the SOOP
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444040201
20240404T200003
Optical aberrations reisduals
Higher noise than usual 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444040202
20240404T203006
Optical aberrations reisduals
Higher noise than usual 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444040204
20240404T213006
Optical aberrations reisduals
Higher noise than usual 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444040205
20240404T220006
Optical aberrations reisduals
Higher noise than usual 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444040208
20240404T233006
Optical aberrations reisduals
Higher noise than usual 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444040207
20240404T230006
Optical aberrations reisduals
Higher noise than usual 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444040203
20240404T210006
Optical aberrations reisduals
Higher noise than usual 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444050201
20240405T200003
Optical aberrations reisduals
Higher noise than usual 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444050202
20240405T203005
Optical aberrations reisduals
Higher noise than usual 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444050203
20240405T210005
Optical aberrations reisduals
Higher noise than usual 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444050206
20240405T223005
Optical aberrations reisduals
Higher noise than usual 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444050204
20240405T213005
Optical aberrations reisduals
Higher noise than usual 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444050207
20240405T230005
Optical aberrations reisduals
Higher noise than usual 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444050205
20240405T220005
Optical aberrations reisduals
Higher noise than usual 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444050208
20240405T233005
Optical aberrations reisduals
Higher noise than usual 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444060201
20240406T200003
Optical aberrations reisduals
Higher noise than usual 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444060202
20240406T203005
Optical aberrations reisduals
Higher noise than usual 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444060203
20240406T210005
Optical aberrations reisduals
Higher noise than usual 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444060204
20240406T213005
Optical aberrations reisduals
Higher noise than usual 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444060208
20240406T233005
Optical aberrations reisduals
Higher noise than usual 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444060205
20240406T220005
Optical aberrations reisduals
Higher noise than usual 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444060207
20240406T230005
Optical aberrations reisduals
Higher noise than usual 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444060206
20240406T223005
Optical aberrations reisduals
Higher noise than usual 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444120101
20240412T010003
Higher noise than usual The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444120102
20240412T014503
Higher noise than usual The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444120104
20240412T224503
Higher noise than usual The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444120103
20240412T220003
Higher noise than usual The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444140102
20240414T014502
Higher noise than usual The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444140101
20240414T010003
Higher noise than usual The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444150101
20240415T010003
Higher noise than usual The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
444150102
20240415T014503
Higher noise than usual The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
449250601
20240925T013009
Optical aberrations reisduals The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
449250603
20240925T080509
Optical aberrations reisduals The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
449250602
20240925T044509
Optical aberrations reisduals The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
449300802
20240930T223710
Optical aberrations reisduals
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The ISS was off during this observation
449300830
20240930T233310
Optical aberrations reisduals
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The ISS was off during this observation
449300808
20240930T224910
Optical aberrations reisduals
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The ISS was off during this observation
449300825
20240930T232310
Optical aberrations reisduals
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The ISS was off during this observation
449300806
20240930T224510
Optical aberrations reisduals
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The ISS was off during this observation
449300814
20240930T230110
Optical aberrations reisduals
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The ISS was off during this observation
449300816
20240930T230510
Optical aberrations reisduals
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The ISS was off during this observation
449300832
20240930T233710
Optical aberrations reisduals
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The ISS was off during this observation
449300810
20240930T225310
Optical aberrations reisduals
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The ISS was off during this observation
449300819
20240930T231110
Optical aberrations reisduals
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The ISS was off during this observation
449300827
20240930T232710
Optical aberrations reisduals
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The ISS was off during this observation
449300813
20240930T225910
Optical aberrations reisduals
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The ISS was off during this observation
449300837
20240930T234710
Optical aberrations reisduals
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The ISS was off during this observation
449300835
20240930T234310
Optical aberrations reisduals
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The ISS was off during this observation
449300831
20240930T233510
Optical aberrations reisduals
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The ISS was off during this observation
449300807
20240930T224710
Optical aberrations reisduals
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The ISS was off during this observation
449300821
20240930T231510
Optical aberrations reisduals
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The ISS was off during this observation
449300828
20240930T232910
Optical aberrations reisduals
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The ISS was off during this observation
449300833
20240930T233910
Optical aberrations reisduals
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The ISS was off during this observation
449300812
20240930T225710
Optical aberrations reisduals
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The ISS was off during this observation
449300836
20240930T234510
Optical aberrations reisduals
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The ISS was off during this observation
449300841
20240930T235510
Optical aberrations reisduals
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The ISS was off during this observation
449300815
20240930T230310
Optical aberrations reisduals
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The ISS was off during this observation
449300840
20240930T235310
Optical aberrations reisduals
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The ISS was off during this observation
449300805
20240930T224310
Optical aberrations reisduals
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The ISS was off during this observation
449300834
20240930T234110
Optical aberrations reisduals
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The ISS was off during this observation
449300820
20240930T231310
Optical aberrations reisduals
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The ISS was off during this observation
449300811
20240930T225510
Optical aberrations reisduals
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The ISS was off during this observation
449300818
20240930T230910
Optical aberrations reisduals
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The ISS was off during this observation
449300824
20240930T232110
Optical aberrations reisduals
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The ISS was off during this observation
449300817
20240930T230710
Optical aberrations reisduals
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The ISS was off during this observation
449300822
20240930T231710
Optical aberrations reisduals
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The ISS was off during this observation
449300804
20240930T224110
Optical aberrations reisduals
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The ISS was off during this observation
449300839
20240930T235110
Optical aberrations reisduals
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The ISS was off during this observation
449300838
20240930T234910
Optical aberrations reisduals
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The ISS was off during this observation
449300809
20240930T225110
Optical aberrations reisduals
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The ISS was off during this observation
449300823
20240930T231910
Optical aberrations reisduals
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The ISS was off during this observation
449300803
20240930T223910
Optical aberrations reisduals
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The ISS was off during this observation
449300826
20240930T232510
Optical aberrations reisduals
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The ISS was off during this observation
449300842
20240930T235710
Optical aberrations reisduals
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The ISS was off during this observation
449300801
20240930T223503
Optical aberrations reisduals
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The ISS was off during this observation
449300829
20240930T233110
Optical aberrations reisduals
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The ISS was off during this observation
449300843
20240930T235910
Optical aberrations reisduals
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The ISS was off during this observation
449300855
20241001T002310
Optical aberrations reisduals
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The ISS was off during this observation
449300854
20241001T002110
Optical aberrations reisduals
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The ISS was off during this observation
449300853
20241001T001910
Optical aberrations reisduals
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The ISS was off during this observation
449300845
20241001T000310
Optical aberrations reisduals
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The ISS was off during this observation
449300852
20241001T001710
Optical aberrations reisduals
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The ISS was off during this observation
449300850
20241001T001310
Optical aberrations reisduals
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The ISS was off during this observation
449300849
20241001T001110
Optical aberrations reisduals
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The ISS was off during this observation
449300846
20241001T000510
Optical aberrations reisduals
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The ISS was off during this observation
449300851
20241001T001510
Optical aberrations reisduals
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The ISS was off during this observation
449300844
20241001T000110
Optical aberrations reisduals
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The ISS was off during this observation
449300860
20241001T003310
Optical aberrations reisduals
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The ISS was off during this observation
449300857
20241001T002710
Optical aberrations reisduals
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The ISS was off during this observation
449300856
20241001T002510
Optical aberrations reisduals
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The ISS was off during this observation
449300848
20241001T000910
Optical aberrations reisduals
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The ISS was off during this observation
449300847
20241001T000710
Optical aberrations reisduals
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The ISS was off during this observation
449300858
20241001T002910
Optical aberrations reisduals
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The ISS was off during this observation
449300859
20241001T003110
Optical aberrations reisduals
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The ISS was off during this observation
450010701
20241001T232607
Few data with ISS off The ISS could not properly correlate during the acquisition of this dataset causing artifacts and higer noise.
450020705
20241002T050107
Few data with ISS off The ISS could not properly correlate during the acquisition of this dataset causing artifacts and higer noise.
450020702
20241002T004610
Few data with ISS off The ISS could not properly correlate during the acquisition of this dataset causing artifacts and higer noise.
450020701
20241002T000607
Few data with ISS off The ISS could not properly correlate during the acquisition of this dataset causing artifacts and higer noise.
450020704
20241002T020107
Few data with ISS off The ISS could not properly correlate during the acquisition of this dataset causing artifacts and higer noise.
450020703
20241002T012610
Few data with ISS off The ISS could not properly correlate during the acquisition of this dataset causing artifacts and higer noise.
450020802
20241002T051313
Optical aberrations reisduals
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The ISS was off during this observation
450020803
20241002T051513
Optical aberrations reisduals
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The ISS was off during this observation
450020807
20241002T052313
Optical aberrations reisduals
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The ISS was off during this observation
450020804
20241002T051713
Optical aberrations reisduals
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The ISS was off during this observation
450020801
20241002T051107
Optical aberrations reisduals
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The ISS was off during this observation
450020806
20241002T052113
Optical aberrations reisduals
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The ISS was off during this observation
450020805
20241002T051913
Optical aberrations reisduals
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The ISS was off during this observation
450020808
20241002T052513
Optical aberrations reisduals
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The ISS was off during this observation
450020809
20241002T052713
Optical aberrations reisduals
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The ISS was off during this observation
450020810
20241002T052913
Optical aberrations reisduals
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The ISS was off during this observation
450020813
20241002T053513
Optical aberrations reisduals
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The ISS was off during this observation
450020812
20241002T053313
Optical aberrations reisduals
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The ISS was off during this observation
450020814
20241002T053713
Optical aberrations reisduals
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The ISS was off during this observation
450020815
20241002T053913
Optical aberrations reisduals
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The ISS was off during this observation
450020816
20241002T054113
Optical aberrations reisduals
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The ISS was off during this observation
450020817
20241002T054313
Optical aberrations reisduals
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The ISS was off during this observation
450020819
20241002T054713
Optical aberrations reisduals
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The ISS was off during this observation
450020825
20241002T055913
Optical aberrations reisduals
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The ISS was off during this observation
450020823
20241002T055513
Optical aberrations reisduals
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The ISS was off during this observation
450020818
20241002T054513
Optical aberrations reisduals
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The ISS was off during this observation
450020822
20241002T055313
Optical aberrations reisduals
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The ISS was off during this observation
450020824
20241002T055713
Optical aberrations reisduals
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The ISS was off during this observation
450020829
20241002T060713
Optical aberrations reisduals
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The ISS was off during this observation
450020827
20241002T060313
Optical aberrations reisduals
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The ISS was off during this observation
450020821
20241002T055113
Optical aberrations reisduals
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The ISS was off during this observation
450020820
20241002T054913
Optical aberrations reisduals
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The ISS was off during this observation
450020826
20241002T060113
Optical aberrations reisduals
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The ISS was off during this observation
450020828
20241002T060513
Optical aberrations reisduals
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The ISS was off during this observation
450020830
20241002T060913
Optical aberrations reisduals
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The ISS was off during this observation
450020811
20241002T053113
Optical aberrations reisduals
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The ISS was off during this observation
450020601
20241002T063105
Dust grain remnants in icnt
AR is cropped 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The AR observed during the acquisition was cropped due to the choice of the pointing.
450020615
20241002T203105
Dust grain remnants in icnt
AR is cropped 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The AR observed during the acquisition was cropped due to the choice of the pointing.
450020616
20241002T213105
Dust grain remnants in icnt
AR is cropped 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The AR observed during the acquisition was cropped due to the choice of the pointing.
450020602
20241002T073100
Dust grain remnants in icnt
AR is cropped 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The AR observed during the acquisition was cropped due to the choice of the pointing.
450020608
20241002T133105
Dust grain remnants in icnt
AR is cropped 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The AR observed during the acquisition was cropped due to the choice of the pointing.
450020611
20241002T163105
Dust grain remnants in icnt
AR is cropped 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The AR observed during the acquisition was cropped due to the choice of the pointing.
450020618
20241002T233104
Dust grain remnants in icnt
AR is cropped 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The AR observed during the acquisition was cropped due to the choice of the pointing.
450020610
20241002T153105
Dust grain remnants in icnt
AR is cropped 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The AR observed during the acquisition was cropped due to the choice of the pointing.
450020609
20241002T143105
Dust grain remnants in icnt
AR is cropped 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The AR observed during the acquisition was cropped due to the choice of the pointing.
450020613
20241002T183105
Dust grain remnants in icnt
AR is cropped 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The AR observed during the acquisition was cropped due to the choice of the pointing.
450020605
20241002T103105
Dust grain remnants in icnt
AR is cropped 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The AR observed during the acquisition was cropped due to the choice of the pointing.
450020606
20241002T113105
Dust grain remnants in icnt
AR is cropped 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The AR observed during the acquisition was cropped due to the choice of the pointing.
450020607
20241002T123105
Dust grain remnants in icnt
AR is cropped 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The AR observed during the acquisition was cropped due to the choice of the pointing.
450020603
20241002T083100
Dust grain remnants in icnt
AR is cropped 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The AR observed during the acquisition was cropped due to the choice of the pointing.
450020617
20241002T223104
Dust grain remnants in icnt
AR is cropped 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The AR observed during the acquisition was cropped due to the choice of the pointing.
450020614
20241002T193105
Dust grain remnants in icnt
AR is cropped 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The AR observed during the acquisition was cropped due to the choice of the pointing.
450020612
20241002T173105
Dust grain remnants in icnt
AR is cropped 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The AR observed during the acquisition was cropped due to the choice of the pointing.
450020604
20241002T093105
Dust grain remnants in icnt
AR is cropped 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The AR observed during the acquisition was cropped due to the choice of the pointing.
450030620
20241003T193104
Dust grain remnants in icnt
AR is cropped 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The AR observed during the acquisition was cropped due to the choice of the pointing.
450030615
20241003T143104
Dust grain remnants in icnt
AR is cropped 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The AR observed during the acquisition was cropped due to the choice of the pointing.
450030606
20241003T053104
Dust grain remnants in icnt
AR is cropped 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The AR observed during the acquisition was cropped due to the choice of the pointing.
450030601
20241003T003104
Dust grain remnants in icnt
AR is cropped 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The AR observed during the acquisition was cropped due to the choice of the pointing.
450030608
20241003T073104
Dust grain remnants in icnt
AR is cropped 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The AR observed during the acquisition was cropped due to the choice of the pointing.
450030619
20241003T183104
Dust grain remnants in icnt
AR is cropped 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The AR observed during the acquisition was cropped due to the choice of the pointing.
450030609
20241003T083100
Dust grain remnants in icnt
AR is cropped 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The AR observed during the acquisition was cropped due to the choice of the pointing.
450030613
20241003T123104
Dust grain remnants in icnt
AR is cropped 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The AR observed during the acquisition was cropped due to the choice of the pointing.
450030605
20241003T043104
Dust grain remnants in icnt
AR is cropped 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The AR observed during the acquisition was cropped due to the choice of the pointing.
450030624
20241003T233104
Dust grain remnants in icnt
AR is cropped 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The AR observed during the acquisition was cropped due to the choice of the pointing.
450030622
20241003T213104
Dust grain remnants in icnt
AR is cropped 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The AR observed during the acquisition was cropped due to the choice of the pointing.
450030610
20241003T093104
Dust grain remnants in icnt
AR is cropped 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The AR observed during the acquisition was cropped due to the choice of the pointing.
450030604
20241003T033104
Dust grain remnants in icnt
AR is cropped 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The AR observed during the acquisition was cropped due to the choice of the pointing.
450030616
20241003T153104
Dust grain remnants in icnt
AR is cropped 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The AR observed during the acquisition was cropped due to the choice of the pointing.
450030614
20241003T133104
Dust grain remnants in icnt
AR is cropped 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The AR observed during the acquisition was cropped due to the choice of the pointing.
450030618
20241003T173104
Dust grain remnants in icnt
AR is cropped 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The AR observed during the acquisition was cropped due to the choice of the pointing.
450030621
20241003T203104
Dust grain remnants in icnt
AR is cropped 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The AR observed during the acquisition was cropped due to the choice of the pointing.
450030607
20241003T063104
Dust grain remnants in icnt
AR is cropped 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The AR observed during the acquisition was cropped due to the choice of the pointing.
450030602
20241003T013104
Dust grain remnants in icnt
AR is cropped 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The AR observed during the acquisition was cropped due to the choice of the pointing.
450030623
20241003T223104
Dust grain remnants in icnt
AR is cropped 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The AR observed during the acquisition was cropped due to the choice of the pointing.
450030603
20241003T023104
Dust grain remnants in icnt
AR is cropped 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The AR observed during the acquisition was cropped due to the choice of the pointing.
450030612
20241003T113104
Dust grain remnants in icnt
AR is cropped 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The AR observed during the acquisition was cropped due to the choice of the pointing.
450030617
20241003T163104
Dust grain remnants in icnt
AR is cropped 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The AR observed during the acquisition was cropped due to the choice of the pointing.
450030611
20241003T103104
Dust grain remnants in icnt
AR is cropped 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The AR observed during the acquisition was cropped due to the choice of the pointing.
450040602
20241004T013104
Dust grain remnants in icnt
AR is cropped 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The AR observed during the acquisition was cropped due to the choice of the pointing.
450040604
20241004T033104
Dust grain remnants in icnt
AR is cropped 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The AR observed during the acquisition was cropped due to the choice of the pointing.
450040605
20241004T043104
Dust grain remnants in icnt
AR is cropped 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The AR observed during the acquisition was cropped due to the choice of the pointing.
450040603
20241004T023104
Dust grain remnants in icnt
AR is cropped 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The AR observed during the acquisition was cropped due to the choice of the pointing.
450040606
20241004T053104
Dust grain remnants in icnt
AR is cropped 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The AR observed during the acquisition was cropped due to the choice of the pointing.
450040601
20241004T003104
Dust grain remnants in icnt
AR is cropped 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The AR observed during the acquisition was cropped due to the choice of the pointing.
450040607
20241004T063104
Dust grain remnants in icnt
AR is cropped 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The AR observed during the acquisition was cropped due to the choice of the pointing.
450040608
20241004T073100
Dust grain remnants in icnt
AR is cropped 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The AR observed during the acquisition was cropped due to the choice of the pointing.
450040611
20241004T103103
Dust grain remnants in icnt
AR is cropped 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The AR observed during the acquisition was cropped due to the choice of the pointing.
450040615
20241004T143103
Dust grain remnants in icnt
AR is cropped 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The AR observed during the acquisition was cropped due to the choice of the pointing.
450040609
20241004T083100
Dust grain remnants in icnt
AR is cropped 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The AR observed during the acquisition was cropped due to the choice of the pointing.
450040612
20241004T113103
Dust grain remnants in icnt
AR is cropped 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The AR observed during the acquisition was cropped due to the choice of the pointing.
450040610
20241004T093103
Dust grain remnants in icnt
AR is cropped 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The AR observed during the acquisition was cropped due to the choice of the pointing.
450040614
20241004T133103
Dust grain remnants in icnt
AR is cropped 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The AR observed during the acquisition was cropped due to the choice of the pointing.
450040613
20241004T123103
Dust grain remnants in icnt
AR is cropped 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The AR observed during the acquisition was cropped due to the choice of the pointing.
450040617
20241004T163103
Dust grain remnants in icnt
AR is cropped 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The AR observed during the acquisition was cropped due to the choice of the pointing.
450040616
20241004T153103
Dust grain remnants in icnt
AR is cropped 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The AR observed during the acquisition was cropped due to the choice of the pointing.
450040618
20241004T173103
Dust grain remnants in icnt
AR is cropped 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The AR observed during the acquisition was cropped due to the choice of the pointing.
450040619
20241004T183103
Dust grain remnants in icnt
AR is cropped 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The AR observed during the acquisition was cropped due to the choice of the pointing.
450040620
20241004T193103
Dust grain remnants in icnt
AR is cropped 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The AR observed during the acquisition was cropped due to the choice of the pointing.
450040621
20241004T203103
Dust grain remnants in icnt
AR is cropped 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The AR observed during the acquisition was cropped due to the choice of the pointing.
450040623
20241004T223103
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
450040622
20241004T213103
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
450040624
20241004T233103
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
450050604
20241005T033104
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
450050601
20241005T003103
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
450050602
20241005T013104
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
450050605
20241005T043103
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
450050608
20241005T073104
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
450050606
20241005T053103
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
450050610
20241005T093103
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
450050609
20241005T083059
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
450050612
20241005T113103
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
450050611
20241005T103103
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
450050613
20241005T123103
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
450050603
20241005T023103
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
450050607
20241005T063103
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
450050614
20241005T133103
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
450050621
20241005T203103
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
450050615
20241005T143103
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
450050619
20241005T183103
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
450050616
20241005T153103
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
450050620
20241005T193103
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
450050623
20241005T223103
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
450050617
20241005T163103
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
450050622
20241005T213103
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
450050618
20241005T173103
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
450050624
20241005T233103
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
450060614
20241006T133102
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
450060607
20241006T063102
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
450060601
20241006T003103
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
450060605
20241006T043102
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
450060616
20241006T153102
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
450060617
20241006T163102
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
450060618
20241006T173102
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
450060621
20241006T203102
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
450060611
20241006T103102
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
450060619
20241006T183102
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
450060609
20241006T083100
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
450060620
20241006T193102
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
450060622
20241006T213102
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
450060602
20241006T013102
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
450060608
20241006T073100
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
450060604
20241006T033102
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
450060603
20241006T023102
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
450060610
20241006T093102
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
450060624
20241006T233102
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
450060612
20241006T113102
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
450060613
20241006T123102
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
450060606
20241006T053102
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
450060615
20241006T143102
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
450060623
20241006T223102
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
450070601
20241007T003102
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
450070607
20241007T063102
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
450070609
20241007T083100
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
450070611
20241007T103102
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
450070604
20241007T033102
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
450070605
20241007T043102
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
450070610
20241007T093102
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
450070602
20241007T013102
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
450070608
20241007T073102
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
450070603
20241007T023102
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
450070612
20241007T113102
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
450070614
20241007T133102
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
450070615
20241007T143102
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
450070617
20241007T163102
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
450070616
20241007T153102
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
450070618
20241007T173102
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
450070621
20241007T203102
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
450070619
20241007T183102
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
450070622
20241007T213102
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
450070623
20241007T223102
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
450070613
20241007T123102
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
450070620
20241007T193102
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
450070624
20241007T233102
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
450080601
20241008T143101
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
450080602
20241008T153101
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
450080603
20241008T163101
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
450080604
20241008T173101
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
450080608
20241008T213101
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
450080605
20241008T183101
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
450080609
20241008T223101
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
450080607
20241008T203101
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
450080606
20241008T193101
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
450080610
20241008T233101
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
450090601
20241009T003101
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
450090602
20241009T013101
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
450090608
20241009T073100
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
450090605
20241009T043101
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
450090604
20241009T033101
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
450090606
20241009T053101
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
450090607
20241009T063101
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
450090610
20241009T093101
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
450090613
20241009T123101
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
450090609
20241009T083100
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
450090611
20241009T103101
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
450090612
20241009T113101
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
450090603
20241009T023101
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
450090614
20241009T133101
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
450090617
20241009T162957
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
450090618
20241009T172956
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
450090615
20241009T143101
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
450090616
20241009T153101
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
450090619
20241009T182957
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
450090623
20241009T222957
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
450090621
20241009T202957
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
450090622
20241009T212957
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
450090624
20241009T232957
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
450090620
20241009T192957
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
450100603
20241010T022957
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
450100601
20241010T002957
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
450100604
20241010T032957
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
450100606
20241010T052957
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
450100602
20241010T012957
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
450100605
20241010T042957
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
450100607
20241010T062957
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
450100620
20241010T192957
Dust grain remnants in icnt
Higher noise than usual
ISS is defocused 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS did not focus causing high noise and artifacts in the data due to random movements of the mirror during the acquisition of eah dataset.
450100613
20241010T122957
Dust grain remnants in icnt
Higher noise than usual
ISS is defocused 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS did not focus causing high noise and artifacts in the data due to random movements of the mirror during the acquisition of eah dataset.
450100616
20241010T152956
Dust grain remnants in icnt
Higher noise than usual
ISS is defocused 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS did not focus causing high noise and artifacts in the data due to random movements of the mirror during the acquisition of eah dataset.
450100618
20241010T172957
Dust grain remnants in icnt
Higher noise than usual
ISS is defocused 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS did not focus causing high noise and artifacts in the data due to random movements of the mirror during the acquisition of eah dataset.
450100612
20241010T112956
Dust grain remnants in icnt
Higher noise than usual
ISS is defocused 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS did not focus causing high noise and artifacts in the data due to random movements of the mirror during the acquisition of eah dataset.
450100624
20241010T232957
Dust grain remnants in icnt
Higher noise than usual
ISS is defocused 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS did not focus causing high noise and artifacts in the data due to random movements of the mirror during the acquisition of eah dataset.
450100619
20241010T182957
Dust grain remnants in icnt
Higher noise than usual
ISS is defocused 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS did not focus causing high noise and artifacts in the data due to random movements of the mirror during the acquisition of eah dataset.
450100615
20241010T142957
Dust grain remnants in icnt
Higher noise than usual
ISS is defocused 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS did not focus causing high noise and artifacts in the data due to random movements of the mirror during the acquisition of eah dataset.
450100622
20241010T212957
Dust grain remnants in icnt
Higher noise than usual
ISS is defocused 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS did not focus causing high noise and artifacts in the data due to random movements of the mirror during the acquisition of eah dataset.
450100609
20241010T082956
Dust grain remnants in icnt
Higher noise than usual
ISS is defocused 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS did not focus causing high noise and artifacts in the data due to random movements of the mirror during the acquisition of eah dataset.
450100610
20241010T092957
Dust grain remnants in icnt
Higher noise than usual
ISS is defocused 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS did not focus causing high noise and artifacts in the data due to random movements of the mirror during the acquisition of eah dataset.
450100623
20241010T222957
Dust grain remnants in icnt
Higher noise than usual
ISS is defocused 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS did not focus causing high noise and artifacts in the data due to random movements of the mirror during the acquisition of eah dataset.
450100621
20241010T202957
Dust grain remnants in icnt
Higher noise than usual
ISS is defocused 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS did not focus causing high noise and artifacts in the data due to random movements of the mirror during the acquisition of eah dataset.
450100611
20241010T102957
Dust grain remnants in icnt
Higher noise than usual
ISS is defocused 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS did not focus causing high noise and artifacts in the data due to random movements of the mirror during the acquisition of eah dataset.
450100614
20241010T132956
Dust grain remnants in icnt
Higher noise than usual
ISS is defocused 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS did not focus causing high noise and artifacts in the data due to random movements of the mirror during the acquisition of eah dataset.
450100617
20241010T162957
Dust grain remnants in icnt
Higher noise than usual
ISS is defocused 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS did not focus causing high noise and artifacts in the data due to random movements of the mirror during the acquisition of eah dataset.
450110607
20241011T062956
Dust grain remnants in icnt
Higher noise than usual
ISS is defocused 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS did not focus causing high noise and artifacts in the data due to random movements of the mirror during the acquisition of eah dataset.
450110608
20241011T072956
Dust grain remnants in icnt
Higher noise than usual
ISS is defocused 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS did not focus causing high noise and artifacts in the data due to random movements of the mirror during the acquisition of eah dataset.
450110609
20241011T082956
Dust grain remnants in icnt
Higher noise than usual
ISS is defocused 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS did not focus causing high noise and artifacts in the data due to random movements of the mirror during the acquisition of eah dataset.
450110606
20241011T052957
Dust grain remnants in icnt
Higher noise than usual
ISS is defocused 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS did not focus causing high noise and artifacts in the data due to random movements of the mirror during the acquisition of eah dataset.
450110602
20241011T012956
Dust grain remnants in icnt
Higher noise than usual
ISS is defocused 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS did not focus causing high noise and artifacts in the data due to random movements of the mirror during the acquisition of eah dataset.
450110604
20241011T032957
Dust grain remnants in icnt
Higher noise than usual
ISS is defocused 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS did not focus causing high noise and artifacts in the data due to random movements of the mirror during the acquisition of eah dataset.
450110603
20241011T022957
Dust grain remnants in icnt
Higher noise than usual
ISS is defocused 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS did not focus causing high noise and artifacts in the data due to random movements of the mirror during the acquisition of eah dataset.
450110605
20241011T042957
Dust grain remnants in icnt
Higher noise than usual
ISS is defocused 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS did not focus causing high noise and artifacts in the data due to random movements of the mirror during the acquisition of eah dataset.
450110601
20241011T002957
Dust grain remnants in icnt
Higher noise than usual
ISS is defocused 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS did not focus causing high noise and artifacts in the data due to random movements of the mirror during the acquisition of eah dataset.
450110612
20241011T112957
Dust grain remnants in icnt
Higher noise than usual
ISS is defocused 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS did not focus causing high noise and artifacts in the data due to random movements of the mirror during the acquisition of eah dataset.
450110610
20241011T092957
Dust grain remnants in icnt
Higher noise than usual
ISS is defocused 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS did not focus causing high noise and artifacts in the data due to random movements of the mirror during the acquisition of eah dataset.
450110613
20241011T122957
Dust grain remnants in icnt
Higher noise than usual
ISS is defocused 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS did not focus causing high noise and artifacts in the data due to random movements of the mirror during the acquisition of eah dataset.
450110614
20241011T132957
Dust grain remnants in icnt
Higher noise than usual
ISS is defocused 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS did not focus causing high noise and artifacts in the data due to random movements of the mirror during the acquisition of eah dataset.
450110615
20241011T142957
Dust grain remnants in icnt
Higher noise than usual
ISS is defocused 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS did not focus causing high noise and artifacts in the data due to random movements of the mirror during the acquisition of eah dataset.
450110611
20241011T102957
Dust grain remnants in icnt
Higher noise than usual
ISS is defocused 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS did not focus causing high noise and artifacts in the data due to random movements of the mirror during the acquisition of eah dataset.
450110617
20241011T162957
Dust grain remnants in icnt
Higher noise than usual
ISS is defocused 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS did not focus causing high noise and artifacts in the data due to random movements of the mirror during the acquisition of eah dataset.
450110616
20241011T152957
Dust grain remnants in icnt
Higher noise than usual
ISS is defocused 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS did not focus causing high noise and artifacts in the data due to random movements of the mirror during the acquisition of eah dataset.
450110619
20241011T182957
Dust grain remnants in icnt
Higher noise than usual
ISS is defocused 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS did not focus causing high noise and artifacts in the data due to random movements of the mirror during the acquisition of eah dataset.
450110618
20241011T172957
Dust grain remnants in icnt
Higher noise than usual
ISS is defocused 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS did not focus causing high noise and artifacts in the data due to random movements of the mirror during the acquisition of eah dataset.
450110621
20241011T202957
Dust grain remnants in icnt
Higher noise than usual
ISS is defocused 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS did not focus causing high noise and artifacts in the data due to random movements of the mirror during the acquisition of eah dataset.
450110620
20241011T192957
Dust grain remnants in icnt
Higher noise than usual
ISS is defocused 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS did not focus causing high noise and artifacts in the data due to random movements of the mirror during the acquisition of eah dataset.
450110622
20241011T212957
Dust grain remnants in icnt
Higher noise than usual
ISS is defocused 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS did not focus causing high noise and artifacts in the data due to random movements of the mirror during the acquisition of eah dataset.
450110623
20241011T222957
Dust grain remnants in icnt
Higher noise than usual
ISS is defocused 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS did not focus causing high noise and artifacts in the data due to random movements of the mirror during the acquisition of eah dataset.
450110624
20241011T232957
Dust grain remnants in icnt
Higher noise than usual
ISS is defocused 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS did not focus causing high noise and artifacts in the data due to random movements of the mirror during the acquisition of eah dataset.
450120602
20241012T012957
Dust grain remnants in icnt
Higher noise than usual
ISS is defocused 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS did not focus causing high noise and artifacts in the data due to random movements of the mirror during the acquisition of eah dataset.
450120601
20241012T002956
Dust grain remnants in icnt
Higher noise than usual
ISS is defocused 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS did not focus causing high noise and artifacts in the data due to random movements of the mirror during the acquisition of eah dataset.
450120605
20241012T042956
Dust grain remnants in icnt
Higher noise than usual
ISS is defocused 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS did not focus causing high noise and artifacts in the data due to random movements of the mirror during the acquisition of eah dataset.
450120607
20241012T062957
Dust grain remnants in icnt
Higher noise than usual
ISS is defocused 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS did not focus causing high noise and artifacts in the data due to random movements of the mirror during the acquisition of eah dataset.
450120604
20241012T032956
Dust grain remnants in icnt
Higher noise than usual
ISS is defocused 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS did not focus causing high noise and artifacts in the data due to random movements of the mirror during the acquisition of eah dataset.
450120603
20241012T022957
Dust grain remnants in icnt
Higher noise than usual
ISS is defocused 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS did not focus causing high noise and artifacts in the data due to random movements of the mirror during the acquisition of eah dataset.
450120606
20241012T052956
Dust grain remnants in icnt
Higher noise than usual
ISS is defocused 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS did not focus causing high noise and artifacts in the data due to random movements of the mirror during the acquisition of eah dataset.
450120608
20241012T072957
Dust grain remnants in icnt
Higher noise than usual
ISS is defocused 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS did not focus causing high noise and artifacts in the data due to random movements of the mirror during the acquisition of eah dataset.
450120609
20241012T082956
Dust grain remnants in icnt
Higher noise than usual
ISS is defocused 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS did not focus causing high noise and artifacts in the data due to random movements of the mirror during the acquisition of eah dataset.
450120610
20241012T092957
Dust grain remnants in icnt
Higher noise than usual
ISS is defocused 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS did not focus causing high noise and artifacts in the data due to random movements of the mirror during the acquisition of eah dataset.
450120612
20241012T112957
Dust grain remnants in icnt
Higher noise than usual
ISS is defocused 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS did not focus causing high noise and artifacts in the data due to random movements of the mirror during the acquisition of eah dataset.
450120611
20241012T102957
Dust grain remnants in icnt
Higher noise than usual
ISS is defocused 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS did not focus causing high noise and artifacts in the data due to random movements of the mirror during the acquisition of eah dataset.
450120613
20241012T122956
Dust grain remnants in icnt
Higher noise than usual
ISS is defocused 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS did not focus causing high noise and artifacts in the data due to random movements of the mirror during the acquisition of eah dataset.
450120614
20241012T132956
Dust grain remnants in icnt
Higher noise than usual
ISS is defocused 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS did not focus causing high noise and artifacts in the data due to random movements of the mirror during the acquisition of eah dataset.
450120615
20241012T142956
Dust grain remnants in icnt
Higher noise than usual
ISS is defocused 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS did not focus causing high noise and artifacts in the data due to random movements of the mirror during the acquisition of eah dataset.
450120617
20241012T162956
Dust grain remnants in icnt
Higher noise than usual
ISS is defocused 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS did not focus causing high noise and artifacts in the data due to random movements of the mirror during the acquisition of eah dataset.
450120618
20241012T172956
Dust grain remnants in icnt
Higher noise than usual
ISS is defocused 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS did not focus causing high noise and artifacts in the data due to random movements of the mirror during the acquisition of eah dataset.
450120619
20241012T182956
Dust grain remnants in icnt
Higher noise than usual
ISS is defocused 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS did not focus causing high noise and artifacts in the data due to random movements of the mirror during the acquisition of eah dataset.
450120616
20241012T152956
Dust grain remnants in icnt
Higher noise than usual
ISS is defocused 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS did not focus causing high noise and artifacts in the data due to random movements of the mirror during the acquisition of eah dataset.
450120620
20241012T192955
Dust grain remnants in icnt
Higher noise than usual
ISS is defocused 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS did not focus causing high noise and artifacts in the data due to random movements of the mirror during the acquisition of eah dataset.
450120621
20241012T202955
Dust grain remnants in icnt
Higher noise than usual
ISS is defocused 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS did not focus causing high noise and artifacts in the data due to random movements of the mirror during the acquisition of eah dataset.
450120624
20241012T232956
Dust grain remnants in icnt
Higher noise than usual
ISS is defocused 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS did not focus causing high noise and artifacts in the data due to random movements of the mirror during the acquisition of eah dataset.
450120623
20241012T222956
Dust grain remnants in icnt
Higher noise than usual
ISS is defocused 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS did not focus causing high noise and artifacts in the data due to random movements of the mirror during the acquisition of eah dataset.
450120622
20241012T212956
Dust grain remnants in icnt
Higher noise than usual
ISS is defocused 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS did not focus causing high noise and artifacts in the data due to random movements of the mirror during the acquisition of eah dataset.
450130606
20241013T052956
Dust grain remnants in icnt
Higher noise than usual
ISS is defocused 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS did not focus causing high noise and artifacts in the data due to random movements of the mirror during the acquisition of eah dataset.
450130603
20241013T022956
Dust grain remnants in icnt
Higher noise than usual
ISS is defocused 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS did not focus causing high noise and artifacts in the data due to random movements of the mirror during the acquisition of eah dataset.
450130602
20241013T012956
Dust grain remnants in icnt
Higher noise than usual
ISS is defocused 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS did not focus causing high noise and artifacts in the data due to random movements of the mirror during the acquisition of eah dataset.
450130605
20241013T042956
Dust grain remnants in icnt
Higher noise than usual
ISS is defocused 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS did not focus causing high noise and artifacts in the data due to random movements of the mirror during the acquisition of eah dataset.
450130601
20241013T002956
Dust grain remnants in icnt
Higher noise than usual
ISS is defocused 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS did not focus causing high noise and artifacts in the data due to random movements of the mirror during the acquisition of eah dataset.
450130609
20241013T082956
Dust grain remnants in icnt
Higher noise than usual
ISS is defocused 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS did not focus causing high noise and artifacts in the data due to random movements of the mirror during the acquisition of eah dataset.
450130604
20241013T032956
Dust grain remnants in icnt
Higher noise than usual
ISS is defocused 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS did not focus causing high noise and artifacts in the data due to random movements of the mirror during the acquisition of eah dataset.
450130611
20241013T102956
Dust grain remnants in icnt
Higher noise than usual
ISS is defocused 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS did not focus causing high noise and artifacts in the data due to random movements of the mirror during the acquisition of eah dataset.
450130608
20241013T072955
Dust grain remnants in icnt
Higher noise than usual
ISS is defocused 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS did not focus causing high noise and artifacts in the data due to random movements of the mirror during the acquisition of eah dataset.
450130607
20241013T062955
Dust grain remnants in icnt
Higher noise than usual
ISS is defocused 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS did not focus causing high noise and artifacts in the data due to random movements of the mirror during the acquisition of eah dataset.
450130610
20241013T092956
Dust grain remnants in icnt
Higher noise than usual
ISS is defocused 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS did not focus causing high noise and artifacts in the data due to random movements of the mirror during the acquisition of eah dataset.
450130612
20241013T112956
Dust grain remnants in icnt
Higher noise than usual
ISS is defocused 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS did not focus causing high noise and artifacts in the data due to random movements of the mirror during the acquisition of eah dataset.
450130613
20241013T122956
Dust grain remnants in icnt
Higher noise than usual
ISS is defocused 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS did not focus causing high noise and artifacts in the data due to random movements of the mirror during the acquisition of eah dataset.
450130614
20241013T132955
Dust grain remnants in icnt
Higher noise than usual
ISS is defocused 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS did not focus causing high noise and artifacts in the data due to random movements of the mirror during the acquisition of eah dataset.
450130624
20241013T232956
Dust grain remnants in icnt
Higher noise than usual
ISS is defocused 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS did not focus causing high noise and artifacts in the data due to random movements of the mirror during the acquisition of eah dataset.
450130619
20241013T182956
Dust grain remnants in icnt
Higher noise than usual
ISS is defocused 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS did not focus causing high noise and artifacts in the data due to random movements of the mirror during the acquisition of eah dataset.
450130623
20241013T222956
Dust grain remnants in icnt
Higher noise than usual
ISS is defocused 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS did not focus causing high noise and artifacts in the data due to random movements of the mirror during the acquisition of eah dataset.
450130622
20241013T212956
Dust grain remnants in icnt
Higher noise than usual
ISS is defocused 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS did not focus causing high noise and artifacts in the data due to random movements of the mirror during the acquisition of eah dataset.
450130620
20241013T192956
Dust grain remnants in icnt
Higher noise than usual
ISS is defocused 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS did not focus causing high noise and artifacts in the data due to random movements of the mirror during the acquisition of eah dataset.
450130616
20241013T152955
Dust grain remnants in icnt
Higher noise than usual
ISS is defocused 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS did not focus causing high noise and artifacts in the data due to random movements of the mirror during the acquisition of eah dataset.
450130621
20241013T202956
Dust grain remnants in icnt
Higher noise than usual
ISS is defocused 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS did not focus causing high noise and artifacts in the data due to random movements of the mirror during the acquisition of eah dataset.
450130615
20241013T142956
Dust grain remnants in icnt
Higher noise than usual
ISS is defocused 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS did not focus causing high noise and artifacts in the data due to random movements of the mirror during the acquisition of eah dataset.
450130618
20241013T172956
Dust grain remnants in icnt
Higher noise than usual
ISS is defocused 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS did not focus causing high noise and artifacts in the data due to random movements of the mirror during the acquisition of eah dataset.
450130617
20241013T162956
Dust grain remnants in icnt
Higher noise than usual
ISS is defocused 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS did not focus causing high noise and artifacts in the data due to random movements of the mirror during the acquisition of eah dataset.
450140601
20241014T002955
Dust grain remnants in icnt
Higher noise than usual
ISS is defocused 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS did not focus causing high noise and artifacts in the data due to random movements of the mirror during the acquisition of eah dataset.
450140603
20241014T022956
Dust grain remnants in icnt
Higher noise than usual
ISS is defocused 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS did not focus causing high noise and artifacts in the data due to random movements of the mirror during the acquisition of eah dataset.
450140604
20241014T032956
Dust grain remnants in icnt
Higher noise than usual
ISS is defocused 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS did not focus causing high noise and artifacts in the data due to random movements of the mirror during the acquisition of eah dataset.
450140605
20241014T042956
Dust grain remnants in icnt
Higher noise than usual
ISS is defocused 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS did not focus causing high noise and artifacts in the data due to random movements of the mirror during the acquisition of eah dataset.
450140602
20241014T012956
Dust grain remnants in icnt
Higher noise than usual
ISS is defocused 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS did not focus causing high noise and artifacts in the data due to random movements of the mirror during the acquisition of eah dataset.
450140606
20241014T052956
Dust grain remnants in icnt
Higher noise than usual
ISS is defocused 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS did not focus causing high noise and artifacts in the data due to random movements of the mirror during the acquisition of eah dataset.
450140607
20241014T062956
Dust grain remnants in icnt
Higher noise than usual
ISS is defocused 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS did not focus causing high noise and artifacts in the data due to random movements of the mirror during the acquisition of eah dataset.
450140613
20241014T122956
Dust grain remnants in icnt
Higher noise than usual
ISS is defocused 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS did not focus causing high noise and artifacts in the data due to random movements of the mirror during the acquisition of eah dataset.
450140610
20241014T092956
Dust grain remnants in icnt
Higher noise than usual
ISS is defocused 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS did not focus causing high noise and artifacts in the data due to random movements of the mirror during the acquisition of eah dataset.
450140620
20241014T192956
Dust grain remnants in icnt
Higher noise than usual
ISS is defocused 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS did not focus causing high noise and artifacts in the data due to random movements of the mirror during the acquisition of eah dataset.
450140618
20241014T172956
Dust grain remnants in icnt
Higher noise than usual
ISS is defocused 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS did not focus causing high noise and artifacts in the data due to random movements of the mirror during the acquisition of eah dataset.
450140614
20241014T132955
Dust grain remnants in icnt
Higher noise than usual
ISS is defocused 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS did not focus causing high noise and artifacts in the data due to random movements of the mirror during the acquisition of eah dataset.
450140619
20241014T182956
Dust grain remnants in icnt
Higher noise than usual
ISS is defocused 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS did not focus causing high noise and artifacts in the data due to random movements of the mirror during the acquisition of eah dataset.
450140616
20241014T152956
Dust grain remnants in icnt
Higher noise than usual
ISS is defocused 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS did not focus causing high noise and artifacts in the data due to random movements of the mirror during the acquisition of eah dataset.
450140611
20241014T102955
Dust grain remnants in icnt
Higher noise than usual
ISS is defocused 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS did not focus causing high noise and artifacts in the data due to random movements of the mirror during the acquisition of eah dataset.
450140609
20241014T082956
Dust grain remnants in icnt
Higher noise than usual
ISS is defocused 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS did not focus causing high noise and artifacts in the data due to random movements of the mirror during the acquisition of eah dataset.
450140623
20241014T222956
Dust grain remnants in icnt
Higher noise than usual
ISS is defocused 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS did not focus causing high noise and artifacts in the data due to random movements of the mirror during the acquisition of eah dataset.
450140622
20241014T212956
Dust grain remnants in icnt
Higher noise than usual
ISS is defocused 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS did not focus causing high noise and artifacts in the data due to random movements of the mirror during the acquisition of eah dataset.
450140612
20241014T112956
Dust grain remnants in icnt
Higher noise than usual
ISS is defocused 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS did not focus causing high noise and artifacts in the data due to random movements of the mirror during the acquisition of eah dataset.
450140615
20241014T142955
Dust grain remnants in icnt
Higher noise than usual
ISS is defocused 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS did not focus causing high noise and artifacts in the data due to random movements of the mirror during the acquisition of eah dataset.
450140608
20241014T072955
Dust grain remnants in icnt
Higher noise than usual
ISS is defocused 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS did not focus causing high noise and artifacts in the data due to random movements of the mirror during the acquisition of eah dataset.
450140621
20241014T202956
Dust grain remnants in icnt
Higher noise than usual
ISS is defocused 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS did not focus causing high noise and artifacts in the data due to random movements of the mirror during the acquisition of eah dataset.
450140624
20241014T232956
Dust grain remnants in icnt
Higher noise than usual
ISS is defocused 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS did not focus causing high noise and artifacts in the data due to random movements of the mirror during the acquisition of eah dataset.
450140617
20241014T162956
Dust grain remnants in icnt
Higher noise than usual
ISS is defocused 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS did not focus causing high noise and artifacts in the data due to random movements of the mirror during the acquisition of eah dataset.
450150701
20241015T180003
Dust grain remnants in icnt
Higher noise than usual
ISS is defocused 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS did not focus causing high noise and artifacts in the data due to random movements of the mirror during the acquisition of eah dataset.
450150601
20241015T002956
Dust grain remnants in icnt
Higher noise than usual
ISS is defocused 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS did not focus causing high noise and artifacts in the data due to random movements of the mirror during the acquisition of eah dataset.
450150603
20241015T022956
Dust grain remnants in icnt
Higher noise than usual
ISS is defocused 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS did not focus causing high noise and artifacts in the data due to random movements of the mirror during the acquisition of eah dataset.
450150602
20241015T012956
Dust grain remnants in icnt
Higher noise than usual
ISS is defocused 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS did not focus causing high noise and artifacts in the data due to random movements of the mirror during the acquisition of eah dataset.
450150701
20241015T180003
ISS off
Dust grain remnants in icnt
Optical aberrations reisduals 		The ISS was off during this observation
Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
450150703
20241015T190003
ISS off
Dust grain remnants in icnt
Optical aberrations reisduals 		The ISS was off during this observation
Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
450150702
20241015T183003
ISS off
Dust grain remnants in icnt
Optical aberrations reisduals 		The ISS was off during this observation
Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
450150704
20241015T193003
ISS off
Dust grain remnants in icnt
Optical aberrations reisduals 		The ISS was off during this observation
Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
450150705
20241015T200003
ISS off
Dust grain remnants in icnt
Optical aberrations reisduals 		The ISS was off during this observation
Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
450150707
20241015T210003
ISS off
Dust grain remnants in icnt
Optical aberrations reisduals 		The ISS was off during this observation
Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
450150706
20241015T203003
ISS off
Dust grain remnants in icnt
Optical aberrations reisduals 		The ISS was off during this observation
Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
450150709
20241015T220003
ISS off
Dust grain remnants in icnt
Optical aberrations reisduals 		The ISS was off during this observation
Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
450150708
20241015T213003
ISS off
Dust grain remnants in icnt
Optical aberrations reisduals 		The ISS was off during this observation
Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
450170733
20241017T224003
Optical aberrations reisduals
Polar Test 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
This observation was meant to be a test for future polar observations with different type of acquisition schemes and pointings.
450170723
20241017T224003
Optical aberrations reisduals
Polar Test 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
This observation was meant to be a test for future polar observations with different type of acquisition schemes and pointings.
450170743
20241017T224003
Optical aberrations reisduals
Polar Test 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
This observation was meant to be a test for future polar observations with different type of acquisition schemes and pointings.
450170701
20241017T220003
Optical aberrations reisduals
Polar Test 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
This observation was meant to be a test for future polar observations with different type of acquisition schemes and pointings.
450170704
20241017T224110
Optical aberrations reisduals
Polar Test 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
This observation was meant to be a test for future polar observations with different type of acquisition schemes and pointings.
450170703
20241017T224003
Optical aberrations reisduals
Polar Test 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
This observation was meant to be a test for future polar observations with different type of acquisition schemes and pointings.
450170706
20241017T224309
Optical aberrations reisduals
Polar Test 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
This observation was meant to be a test for future polar observations with different type of acquisition schemes and pointings.
450170707
20241017T224409
Optical aberrations reisduals
Polar Test 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
This observation was meant to be a test for future polar observations with different type of acquisition schemes and pointings.
450170705
20241017T224209
Optical aberrations reisduals
Polar Test 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
This observation was meant to be a test for future polar observations with different type of acquisition schemes and pointings.
450170709
20241017T224609
Optical aberrations reisduals
Polar Test 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
This observation was meant to be a test for future polar observations with different type of acquisition schemes and pointings.
450170708
20241017T224509
Optical aberrations reisduals
Polar Test 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
This observation was meant to be a test for future polar observations with different type of acquisition schemes and pointings.
450170710
20241017T224709
Optical aberrations reisduals
Polar Test 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
This observation was meant to be a test for future polar observations with different type of acquisition schemes and pointings.
450170711
20241017T224809
Optical aberrations reisduals
Polar Test 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
This observation was meant to be a test for future polar observations with different type of acquisition schemes and pointings.
450170712
20241017T224909
Optical aberrations reisduals
Polar Test 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
This observation was meant to be a test for future polar observations with different type of acquisition schemes and pointings.
450170713
20241017T230003
Optical aberrations reisduals
Polar Test 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
This observation was meant to be a test for future polar observations with different type of acquisition schemes and pointings.
450170715
20241017T230209
Optical aberrations reisduals
Polar Test 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
This observation was meant to be a test for future polar observations with different type of acquisition schemes and pointings.
450170714
20241017T230109
Optical aberrations reisduals
Polar Test 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
This observation was meant to be a test for future polar observations with different type of acquisition schemes and pointings.
450170718
20241017T233003
Optical aberrations reisduals
Polar Test 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
This observation was meant to be a test for future polar observations with different type of acquisition schemes and pointings.
450170716
20241017T230309
Optical aberrations reisduals
Polar Test 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
This observation was meant to be a test for future polar observations with different type of acquisition schemes and pointings.
450170717
20241017T230409
Optical aberrations reisduals
Polar Test 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
This observation was meant to be a test for future polar observations with different type of acquisition schemes and pointings.
450180753
20241018T000503
Optical aberrations reisduals
Polar Test 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
This observation was meant to be a test for future polar observations with different type of acquisition schemes and pointings.
450180763
20241018T000503
Optical aberrations reisduals
Polar Test 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
This observation was meant to be a test for future polar observations with different type of acquisition schemes and pointings.
450180744
20241018T001149
Optical aberrations reisduals
Polar Test 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
This observation was meant to be a test for future polar observations with different type of acquisition schemes and pointings.
450180743
20241018T001009
Optical aberrations reisduals
Polar Test 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
This observation was meant to be a test for future polar observations with different type of acquisition schemes and pointings.
450180740
20241018T000503
Optical aberrations reisduals
Polar Test 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
This observation was meant to be a test for future polar observations with different type of acquisition schemes and pointings.
450180749
20241018T004503
Optical aberrations reisduals
Polar Test 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
This observation was meant to be a test for future polar observations with different type of acquisition schemes and pointings.
450180746
20241018T001509
Optical aberrations reisduals
Polar Test 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
This observation was meant to be a test for future polar observations with different type of acquisition schemes and pointings.
450180747
20241018T001649
Optical aberrations reisduals
Polar Test 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
This observation was meant to be a test for future polar observations with different type of acquisition schemes and pointings.
450180741
20241018T000649
Optical aberrations reisduals
Polar Test 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
This observation was meant to be a test for future polar observations with different type of acquisition schemes and pointings.
450180742
20241018T000829
Optical aberrations reisduals
Polar Test 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
This observation was meant to be a test for future polar observations with different type of acquisition schemes and pointings.
450180745
20241018T001329
Optical aberrations reisduals
Polar Test 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
This observation was meant to be a test for future polar observations with different type of acquisition schemes and pointings.
450180751
20241018T004829
Optical aberrations reisduals
Polar Test 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
This observation was meant to be a test for future polar observations with different type of acquisition schemes and pointings.
450180750
20241018T004649
Optical aberrations reisduals
Polar Test 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
This observation was meant to be a test for future polar observations with different type of acquisition schemes and pointings.
450190702
20241019T190110
Optical aberrations reisduals
Higher noise than usual
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS was off during this observation
450190701
20241019T190003
Optical aberrations reisduals
Higher noise than usual
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS was off during this observation
450190703
20241019T190210
Optical aberrations reisduals
Higher noise than usual
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS was off during this observation
450190704
20241019T190310
Optical aberrations reisduals
Higher noise than usual
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS was off during this observation
450190707
20241019T190610
Optical aberrations reisduals
Higher noise than usual
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS was off during this observation
450190705
20241019T190410
Optical aberrations reisduals
Higher noise than usual
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS was off during this observation
450190709
20241019T190810
Optical aberrations reisduals
Higher noise than usual
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS was off during this observation
450190712
20241019T191110
Optical aberrations reisduals
Higher noise than usual
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS was off during this observation
450190706
20241019T190510
Optical aberrations reisduals
Higher noise than usual
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS was off during this observation
450190718
20241019T191710
Optical aberrations reisduals
Higher noise than usual
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS was off during this observation
450190713
20241019T191210
Optical aberrations reisduals
Higher noise than usual
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS was off during this observation
450190708
20241019T190709
Optical aberrations reisduals
Higher noise than usual
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS was off during this observation
450190717
20241019T191610
Optical aberrations reisduals
Higher noise than usual
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS was off during this observation
450190722
20241019T192110
Optical aberrations reisduals
Higher noise than usual
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS was off during this observation
450190710
20241019T190910
Optical aberrations reisduals
Higher noise than usual
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS was off during this observation
450190719
20241019T191810
Optical aberrations reisduals
Higher noise than usual
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS was off during this observation
450190721
20241019T192010
Optical aberrations reisduals
Higher noise than usual
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS was off during this observation
450190711
20241019T191010
Optical aberrations reisduals
Higher noise than usual
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS was off during this observation
450190730
20241019T192910
Optical aberrations reisduals
Higher noise than usual
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS was off during this observation
450190715
20241019T191410
Optical aberrations reisduals
Higher noise than usual
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS was off during this observation
450190724
20241019T192310
Optical aberrations reisduals
Higher noise than usual
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS was off during this observation
450190728
20241019T192710
Optical aberrations reisduals
Higher noise than usual
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS was off during this observation
450190729
20241019T192810
Optical aberrations reisduals
Higher noise than usual
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS was off during this observation
450190723
20241019T192210
Optical aberrations reisduals
Higher noise than usual
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS was off during this observation
450190716
20241019T191510
Optical aberrations reisduals
Higher noise than usual
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS was off during this observation
450190734
20241019T193310
Optical aberrations reisduals
Higher noise than usual
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS was off during this observation
450190725
20241019T192410
Optical aberrations reisduals
Higher noise than usual
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS was off during this observation
450190714
20241019T191310
Optical aberrations reisduals
Higher noise than usual
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS was off during this observation
450190732
20241019T193110
Optical aberrations reisduals
Higher noise than usual
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS was off during this observation
450190727
20241019T192610
Optical aberrations reisduals
Higher noise than usual
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS was off during this observation
450190731
20241019T193010
Optical aberrations reisduals
Higher noise than usual
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS was off during this observation
450190720
20241019T191910
Optical aberrations reisduals
Higher noise than usual
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS was off during this observation
450190726
20241019T192510
Optical aberrations reisduals
Higher noise than usual
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS was off during this observation
450190735
20241019T193410
Optical aberrations reisduals
Higher noise than usual
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS was off during this observation
450190733
20241019T193210
Optical aberrations reisduals
Higher noise than usual
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS was off during this observation
450190736
20241019T193510
Optical aberrations reisduals
Higher noise than usual
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS was off during this observation
450190739
20241019T193810
Optical aberrations reisduals
Higher noise than usual
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS was off during this observation
450190737
20241019T193610
Optical aberrations reisduals
Higher noise than usual
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS was off during this observation
450190738
20241019T193710
Optical aberrations reisduals
Higher noise than usual
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS was off during this observation
450190740
20241019T193910
Optical aberrations reisduals
Higher noise than usual
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS was off during this observation
450190742
20241019T194110
Optical aberrations reisduals
Higher noise than usual
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS was off during this observation
450190741
20241019T194010
Optical aberrations reisduals
Higher noise than usual
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS was off during this observation
450190745
20241019T194410
Optical aberrations reisduals
Higher noise than usual
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS was off during this observation
450190743
20241019T194210
Optical aberrations reisduals
Higher noise than usual
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS was off during this observation
450190744
20241019T194310
Optical aberrations reisduals
Higher noise than usual
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS was off during this observation
450190747
20241019T194610
Optical aberrations reisduals
Higher noise than usual
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS was off during this observation
450190746
20241019T194510
Optical aberrations reisduals
Higher noise than usual
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS was off during this observation
450190749
20241019T194810
Optical aberrations reisduals
Higher noise than usual
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS was off during this observation
450190748
20241019T194710
Optical aberrations reisduals
Higher noise than usual
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS was off during this observation
450190750
20241019T194910
Optical aberrations reisduals
Higher noise than usual
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS was off during this observation
450190751
20241019T195010
Optical aberrations reisduals
Higher noise than usual
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS was off during this observation
450190752
20241019T195110
Optical aberrations reisduals
Higher noise than usual
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS was off during this observation
450190753
20241019T195210
Optical aberrations reisduals
Higher noise than usual
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS was off during this observation
450190755
20241019T195410
Optical aberrations reisduals
Higher noise than usual
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS was off during this observation
450190754
20241019T195310
Optical aberrations reisduals
Higher noise than usual
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS was off during this observation
450190756
20241019T195510
Optical aberrations reisduals
Higher noise than usual
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS was off during this observation
450190758
20241019T195710
Optical aberrations reisduals
Higher noise than usual
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS was off during this observation
450190757
20241019T195610
Optical aberrations reisduals
Higher noise than usual
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS was off during this observation
450190759
20241019T195810
Optical aberrations reisduals
Higher noise than usual
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS was off during this observation
450190760
20241019T195910
Optical aberrations reisduals
Higher noise than usual
ISS off 		The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
The ISS was off during this observation
450200102
20241020T070003
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
450200101
20241020T050003
Dust grain remnants in icnt Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
470220101
20241022T032803
Inaccurate prefilter correction The prefilter correction is not perfect at the edge of the field of view causing problems in some of the RTE results.
470220102
20241022T033903
Inaccurate prefilter correction The prefilter correction is not perfect at the edge of the field of view causing problems in some of the RTE results.
470220104
20241022T040103
Inaccurate prefilter correction The prefilter correction is not perfect at the edge of the field of view causing problems in some of the RTE results.
470220103
20241022T035003
Inaccurate prefilter correction The prefilter correction is not perfect at the edge of the field of view causing problems in some of the RTE results.
470220106
20241022T042303
Inaccurate prefilter correction The prefilter correction is not perfect at the edge of the field of view causing problems in some of the RTE results.
470220105
20241022T041203
Inaccurate prefilter correction The prefilter correction is not perfect at the edge of the field of view causing problems in some of the RTE results.
470220108
20241022T044503
Inaccurate prefilter correction The prefilter correction is not perfect at the edge of the field of view causing problems in some of the RTE results.
470220107
20241022T043403
Inaccurate prefilter correction The prefilter correction is not perfect at the edge of the field of view causing problems in some of the RTE results.
470220111
20241022T051803
Inaccurate prefilter correction The prefilter correction is not perfect at the edge of the field of view causing problems in some of the RTE results.
470220113
20241022T054003
Inaccurate prefilter correction The prefilter correction is not perfect at the edge of the field of view causing problems in some of the RTE results.
470220114
20241022T055103
Inaccurate prefilter correction The prefilter correction is not perfect at the edge of the field of view causing problems in some of the RTE results.
470220110
20241022T050703
Inaccurate prefilter correction The prefilter correction is not perfect at the edge of the field of view causing problems in some of the RTE results.
470220109
20241022T045603
Inaccurate prefilter correction The prefilter correction is not perfect at the edge of the field of view causing problems in some of the RTE results.
470220112
20241022T052903
Inaccurate prefilter correction The prefilter correction is not perfect at the edge of the field of view causing problems in some of the RTE results.
470220119
20241022T064603
Inaccurate prefilter correction The prefilter correction is not perfect at the edge of the field of view causing problems in some of the RTE results.
470220117
20241022T062403
Inaccurate prefilter correction The prefilter correction is not perfect at the edge of the field of view causing problems in some of the RTE results.
470220115
20241022T060203
Inaccurate prefilter correction The prefilter correction is not perfect at the edge of the field of view causing problems in some of the RTE results.
470220116
20241022T061303
Inaccurate prefilter correction The prefilter correction is not perfect at the edge of the field of view causing problems in some of the RTE results.
470220118
20241022T063503
Inaccurate prefilter correction The prefilter correction is not perfect at the edge of the field of view causing problems in some of the RTE results.
470220121
20241022T070803
Inaccurate prefilter correction The prefilter correction is not perfect at the edge of the field of view causing problems in some of the RTE results.
470220122
20241022T071903
Inaccurate prefilter correction The prefilter correction is not perfect at the edge of the field of view causing problems in some of the RTE results.
470220120
20241022T065703
Inaccurate prefilter correction The prefilter correction is not perfect at the edge of the field of view causing problems in some of the RTE results.
470220124
20241022T074103
Inaccurate prefilter correction The prefilter correction is not perfect at the edge of the field of view causing problems in some of the RTE results.
470220123
20241022T073003
Inaccurate prefilter correction The prefilter correction is not perfect at the edge of the field of view causing problems in some of the RTE results.
470220125
20241022T075203
Inaccurate prefilter correction The prefilter correction is not perfect at the edge of the field of view causing problems in some of the RTE results.
450220702
20241022T090503
Dust grain remnants in icnt
Inaccurate prefilter correction 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The prefilter correction is not perfect at the edge of the field of view causing problems in some of the RTE results.
450220705
20241022T093503
Dust grain remnants in icnt
Inaccurate prefilter correction 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The prefilter correction is not perfect at the edge of the field of view causing problems in some of the RTE results.
450220704
20241022T092503
Dust grain remnants in icnt
Inaccurate prefilter correction 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The prefilter correction is not perfect at the edge of the field of view causing problems in some of the RTE results.
450220703
20241022T091503
Dust grain remnants in icnt
Inaccurate prefilter correction 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The prefilter correction is not perfect at the edge of the field of view causing problems in some of the RTE results.
450220706
20241022T094503
Dust grain remnants in icnt
Inaccurate prefilter correction 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The prefilter correction is not perfect at the edge of the field of view causing problems in some of the RTE results.
450220701
20241022T085503
Dust grain remnants in icnt
Inaccurate prefilter correction 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The prefilter correction is not perfect at the edge of the field of view causing problems in some of the RTE results.
450230706
20241023T094504
Dust grain remnants in icnt
Inaccurate prefilter correction 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The prefilter correction is not perfect at the edge of the field of view causing problems in some of the RTE results.
450230704
20241023T092504
Dust grain remnants in icnt
Inaccurate prefilter correction 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The prefilter correction is not perfect at the edge of the field of view causing problems in some of the RTE results.
450230702
20241023T090504
Dust grain remnants in icnt
Inaccurate prefilter correction 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The prefilter correction is not perfect at the edge of the field of view causing problems in some of the RTE results.
450230705
20241023T093504
Dust grain remnants in icnt
Inaccurate prefilter correction 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The prefilter correction is not perfect at the edge of the field of view causing problems in some of the RTE results.
450230703
20241023T091504
Dust grain remnants in icnt
Inaccurate prefilter correction 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The prefilter correction is not perfect at the edge of the field of view causing problems in some of the RTE results.
450230701
20241023T085503
Dust grain remnants in icnt
Inaccurate prefilter correction 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The prefilter correction is not perfect at the edge of the field of view causing problems in some of the RTE results.
450240601
20241024T035003
Dust grain remnants in icnt
Optical aberrations reisduals 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
450240604
20241024T040804
Dust grain remnants in icnt
Optical aberrations reisduals 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
450240603
20241024T040204
Dust grain remnants in icnt
Optical aberrations reisduals 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
450240602
20241024T035604
Dust grain remnants in icnt
Optical aberrations reisduals 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
450240608
20241024T043204
Dust grain remnants in icnt
Optical aberrations reisduals 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
450240605
20241024T041404
Dust grain remnants in icnt
Optical aberrations reisduals 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
450240607
20241024T042604
Dust grain remnants in icnt
Optical aberrations reisduals 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
450240609
20241024T043804
Dust grain remnants in icnt
Optical aberrations reisduals 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
450240606
20241024T042004
Dust grain remnants in icnt
Optical aberrations reisduals 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
450240610
20241024T044404
Dust grain remnants in icnt
Optical aberrations reisduals 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
450240701
20241024T111713
Dust grain remnants in icnt
Optical aberrations reisduals 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
450240702
20241024T112714
Dust grain remnants in icnt
Optical aberrations reisduals 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
450240703
20241024T113714
Dust grain remnants in icnt
Optical aberrations reisduals 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
450240704
20241024T114714
Dust grain remnants in icnt
Optical aberrations reisduals 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
450240705
20241024T115714
Dust grain remnants in icnt
Optical aberrations reisduals 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
450240706
20241024T120714
Dust grain remnants in icnt
Optical aberrations reisduals 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
450240302
20241024T192003
Dust grain remnants in icnt
Optical aberrations reisduals
Higher noise than usual 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
450240303
20241024T230503
Dust grain remnants in icnt
Optical aberrations reisduals
Higher noise than usual 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
450240301
20241024T160003
Dust grain remnants in icnt
Optical aberrations reisduals
Higher noise than usual 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
450250301
20241025T025003
Dust grain remnants in icnt
Optical aberrations reisduals
Higher noise than usual 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
450250302
20241025T062003
Dust grain remnants in icnt
Optical aberrations reisduals
Higher noise than usual 		Residuals of one or more dust grains are still visible in the continuum intensity and slightly in the magnetic and velocity fields
The PSF deconvolution did not remove completely the optical aberrations. Weak residual aberrations may be visible.
The noise level in this dataset is higher than in usual datasets because of the instrumental conditions during the acquisition.
Contact: Julian Blanco - SOPHI Support
Universitat de Valencia 2022