A dataset provided by the European Space Agency

Name 9370
Title The Optical Counterpart of an Ultraluminous X-Ray Source
URL https://hst.esac.esa.int/ehst/#/pages/search;proposal=9370;TAPCLIENT=DOI
DOI https://doi.org/10.5270/esa-69fko2f
Author Bregman, Joel N.
Description This is a scientific proposal for HST mission. For specific information please visit https://archive.stsci.edu/proposal_search.php?id=9370&mission=hst
Publication
  • Compact Optical Counterparts of Ultraluminous X-Ray Sources
  • Irradiation models for ULXs and fits to optical data
  • Optical Counterparts of the Nearest Ultraluminous X-Ray Sources
  • Roche-lobe Overflow Systems Powered by Black Holes in Young Star Clusters: The Importance of Dynamical Exchanges
  • The impact of satellite trails on Hubble Space Telescope observations
  • The Optical Counterpart of an Ultraluminous X-Ray Source in NGC 5204
  • Ultra-luminous X-ray sources
Instrument ACS, ACS/HRC, ACS/WFC, STIS, STIS/CCD, STIS/FUV-MAMA
Temporal Coverage 2002-10-28T23:45:57Z/2002-11-24T19:04:36Z
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 2003-11-24T19:04:36Z
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, Bregman comma Joel N., 2003, 'The Optical Counterpart of an Ultraluminous X-Ray Source', 1.0, European Space Agency, https://doi.org/10.5270/esa-69fko2f