A dataset provided by the European Space Agency

Name 11642
Title FUV/X-ray absorption and emission line spectroscopy of the Galactic corona
URL https://hst.esac.esa.int/ehst/#/pages/search;proposal=11642;TAPCLIENT=DOI
DOI https://doi.org/10.5270/esa-1oxyl45
Author Yao, Yangsen
Description This is a scientific proposal for HST mission. For specific information please visit https://archive.stsci.edu/proposal_search.php?id=11642&mission=hst
Publication
  • High-resolution ultraviolet spectroscopy of gas in galaxy halos and large-scale structures
  • Measuring the black hole masses in accreting X-ray binaries by detecting the Doppler orbital motion of their accretion disc wind absorption lines
  • Variable O VI and N V Emission from the X-ray Binary LMC X-3: Heating of the Black Hole Companion
Instrument COS, COS/FUV, COS/NUV
Temporal Coverage 2009-12-15T03:44:14Z/2009-12-15T13:16:49Z
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 2010-12-15T16:51:17Z
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, Yao comma Yangsen, 2010, 'FUV/X-ray absorption and emission line spectroscopy of the Galactic corona', 1.0, European Space Agency, https://doi.org/10.5270/esa-1oxyl45