Astrometry with Hubble Space Telescope Fine Guidance Sensors--A Review
Hubble Space Telescope Fine Guidance Sensor Astrometric Parallaxesfor Three Dwarf Novae: SS Aurigae, SS Cygni, and U Geminorum
On the Hubble Space Telescope Trigonometric Parallax of the Dwarf Nova SS Cygni
The dwarf nova SS Cygni: what is wrong?
The Spectroscopic and Astrometric Parallaxes of Three Dwarf Novae: The Nature of the Secondary Stars of U Geminorum, SS Aurigae, and SS Cygni
Instrument
FGS
Temporal Coverage
1998-03-14T10:42:11Z/1998-12-17T03:09:25Z
Version
1.0
Mission Description
Launched in 1990, the NASA/ESA Hubble Space Telescope remains the premier UV and visible light telescope in orbit. With well over 1.6 million observations from 10 different scientific instruments, the ESA Hubble Science Archive is a treasure trove of astronomical data to be exploited.
European Space Agency, Harrison comma Thomas, 1999, 'The Distances to Dwarf Novae, and the Calibration of the Technique of Infrared Spectroscopic Parallax', 1.0, European Space Agency, https://doi.org/10.57780/esa-l6fo3qd