Group Research
- Radiosupernovae.
- Quasars and Active Galactic Nuclei.
- High Precission Differential
Astrometry.
- Radiostars.
- Gravitational Lenses.
- New Instruments (ALMA, SKA).
MAIN CONTRIBUTIONS
Radiosupernovae
Discovery of the first
shell-like radiosupernova structure (Marcaide
et al. Nature, 373, 44, 1995).
First film of a supernova expansion (Marcaide et al. Science, 270, 1475, 1995).
(Movie of the SN1993J supernova expansion)
(Images of the SN1993J expansion through 10 years)
(Images of the SN1993J expansion published in Science)
First determination of deceleration in the expansion of a supernova (Marcaide et al. ApJL, 486, L31, 1997).
Creation of a supernovae radio emission simultation code (Pérez-Torres, Alberdi y Marcaide, A&A, 374, 997, 2001).
High Precission Astrometry
First detection of the low
mass companion of a radiostar by astrometric methods (Guirado
et al., ApJ, 490, 835, 1997).
Demonstration of the possibility of making High Precission Differential Astrometry in high resolution VLBI observations, as much at millimeter wavelengths (Guirado et al., A&A, 353, L37, 2000) as with space antennas, using the HALCA japanese satellite of the VSOP project (Guirado et al., A&A, 371, 766, 2001).
Gravitational Lenses
Determination of the mass
distribution and identification of a new galaxy in the MGJ0414+0534
quad lens, solving a previous disagreement of other researchers, with
the highest quality VLBI observations ever obtained of the source.