A dataset provided by the European Space Agency

Name 12010
Title COS FUV Line Spread Function Characterization
URL https://hst.esac.esa.int/ehst/#/pages/search;proposal=12010;TAPCLIENT=DOI
DOI https://doi.org/10.5270/esa-xwbhyjx
Author Ghavamian, Parviz
Description This is a scientific proposal for HST mission. For specific information please visit https://archive.stsci.edu/proposal_search.php?id=12010&mission=hst
Publication
  • Optical Emission of the Ultraluminous X-Ray Source NGC 5408 X-1: Donor Star or Irradiated Accretion Disk?
  • Optically thick structure in early B-type supergiant stellar winds at low metallicities
  • Thermal stability of winds driven by radiation pressure in super-Eddington accretion discs
Instrument STIS, STIS/CCD, STIS/FUV-MAMA
Temporal Coverage 2009-09-23T21:25:05Z/2009-09-23T23:50:39Z
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 2009-09-24T03:45:34Z
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, Ghavamian et al., 2009, 'COS FUV Line Spread Function Characterization', 1.0, European Space Agency, https://doi.org/10.5270/esa-xwbhyjx