Astrometry with Hubble Space Telescope Fine Guidance Sensors--A Review
How to Constrain Your M Dwarf. II. The Mass-Luminosity-Metallicity Relation from 0.075 to 0.70 Solar Masses
Interferometric Astrometry of Proxima Centauri and Barnards Star Using HUBBLE SPACE TELESCOPE Fine Guidance Sensor 3: Detection Limits for Substellar Companions
Interferometric Astrometry of the Low-Mass Binary GL 791.2 (= HU Del) UsingHubble Space Telescope Fine Guidance Sensor 3: Parallax and Component Masses
Stellar and substellar companions of nearby stars from Gaia DR2. Binarity from proper motion anomaly
The Solar Neighborhood. XXXVII: The Mass-Luminosity Relation for Main-sequence M Dwarfs
Instrument
FGS
Temporal Coverage
1995-08-20T16:14:23Z/1996-06-20T18:27:01Z
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, Benedict comma George Fritz, 1997, 'DETECTION AND MASS DETERMINATION OF LOW-MASS COMPANIONS TO NEARBY M DWARFS', 1.0, European Space Agency, https://doi.org/10.57780/esa-eovb4eq