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
Precise Masses for Wolf 1062 AB from Hubble Space Telescope Interferometric Astrometry and MCDonald Observatory Radial Velocities
The First Definitive Binary Orbit Determined with the Hubble Space Telescope Fine Guidance Sensors: Wolf 1062 (Gliese 748)
The Nearby Low-Mass Visual Binary Wolf 424
The Optical Mass-Luminosity Relation at the End of the Main Sequence (0.08-0.20 Msolar)
The Solar Neighborhood. XXXVII: The Mass-Luminosity Relation for Main-sequence M Dwarfs
Instrument
FGS
Temporal Coverage
1995-07-24T02:33:00Z/1997-02-02T00:00:51Z
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, Henry comma Todd J., 1998, 'Calibrating the Mass-Luminosity Relation at the End of the Main Sequence', 1.0, European Space Agency, https://doi.org/10.57780/esa-a88iofx