A dataset provided by the European Space Agency

Name 6345
Title Determining the Binary Frequency for Ultra-cool, Nearby M Dwarfs
URL https://hst.esac.esa.int/ehst/#/pages/search;proposal=6345;TAPCLIENT=DOI
DOI https://doi.org/10.5270/esa-6qe376w
Author Kirkpatrick, J. Davy
Description This is a scientific proposal for HST mission. For specific information please visit https://archive.stsci.edu/proposal_search.php?id=6345&mission=hst
Publication
  • Direct measurements of the fundamental properties of low-mass stars and brown dwarfs
  • Discovery of a Tight Brown Dwarf Companion to theLow-Mass Star LHS 2397a
  • First NACO observations of the Brown Dwarf LHS 2397aB
  • Individual Dynamical Masses of Ultracool Dwarfs
  • Keck Laser Guide Star Adaptive Optics Monitoring of the M8+L7 Binary LHS 2397aAB: First Dynamical Mass Benchmark at the L/T Transition
Instrument WFPC2, WFPC2/PC
Temporal Coverage 1996-01-09T10:21:15Z/1997-05-05T01:37:14Z
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 1998-05-05T10:14:26Z
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, Kirkpatrick et al., 1998, 'Determining the Binary Frequency for Ultra-cool, Nearby M Dwarfs', 1.0, European Space Agency, https://doi.org/10.5270/esa-6qe376w