A dataset provided by the European Space Agency

Name 7493
Title Calibrating the Mass-Luminosity Relation at the End of the Main Sequence
URL https://hst.esac.esa.int/ehst/#/pages/search;proposal=7493;TAPCLIENT=DOI
DOI https://doi.org/10.57780/esa-k42vdjx
Author Henry, Todd J.
Description This is a scientific proposal for HST mission. For specific information please visit https://archive.stsci.edu/proposal_search.php?id=7493&mission=hst
Publication
  • 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
  • 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. XLV. The Stellar Multiplicity Rate of M Dwarfs Within 25 pc
  • The Solar Neighborhood. XXXVII: The Mass-Luminosity Relation for Main-sequence M Dwarfs
Instrument FGS
Temporal Coverage 1997-09-16T14:24:28Z/1998-05-31T22:54:43Z
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.
Creator Contact https://support.cosmos.esa.int/esdc/index.php?/Tickets/Submit
Date Published 1999-06-02T13:27:52Z
Last Update 2025-01-25
Keywords Hubble, HST, HLA, HCV, ACS, COS, STIS, WFC3, FOC, FOS, HRS, NICMOS, WFPC, WFPC2
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, Henry et al., 1999, 'Calibrating the Mass-Luminosity Relation at the End of the Main Sequence', 1.0, European Space Agency, https://doi.org/10.57780/esa-k42vdjx