A dataset provided by the European Space Agency

Name 6677
Title The Origin of the X-Ray Background: What are the faintest X-Ray Galaxies?
URL https://hst.esac.esa.int/ehst/#/pages/search;proposal=6677;TAPCLIENT=DOI
DOI https://doi.org/10.5270/esa-jz9eylu
Author McHardy, Ian M.
Description This is a scientific proposal for HST mission. For specific information please visit https://archive.stsci.edu/proposal_search.php?id=6677&mission=hst
Publication
  • Merger-driven Growth of Intermediate-mass Black Holes: Constraints from Hubble Space Telescope Imaging of Hyper-luminous X-Ray Sources
Instrument WFPC2, WFPC2/PC, WFPC2/WFC
Temporal Coverage 1997-03-29T17:06:14Z/1998-11-01T22:53:14Z
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 1999-11-02T16:02:07Z
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, McHardy et al., 1999, 'The Origin of the X-Ray Background: What are the faintest X-Ray Galaxies?', 1.0, European Space Agency, https://doi.org/10.5270/esa-jz9eylu