A dataset provided by the European Space Agency

Name 6696
Title STUDYING THE UV EMISSION LINE SPECTRUM OF HIGH Z RADIO GALAXIES. EFFECTS OF GEOMETRY AND DUST.
URL https://hst.esac.esa.int/ehst/#/pages/search;proposal=6696;TAPCLIENT=DOI
DOI https://doi.org/10.5270/esa-fdsji56
Author Fosbury, Robert
Description This is a scientific proposal for HST mission. For specific information please visit https://archive.stsci.edu/proposal_search.php?id=6696&mission=hst
Publication
  • A Relation between Supermassive Black Hole Mass and Quasar Metallicity?
  • Emission Line Properties of Active Galactic Nuclei from a Post-COSTAR Hubble Space Telescope Faint Object Spectrograph Spectral Atlas
Instrument FOS/BL, FOS/RD
Temporal Coverage 1996-09-19T10:24:21Z/1996-10-01T18:43:12Z
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 1997-10-02T03:00:20Z
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, Fosbury comma Robert, 1997, 'STUDYING THE UV EMISSION LINE SPECTRUM OF HIGH Z RADIO GALAXIES. EFFECTS OF GEOMETRY AND DUST.', 1.0, European Space Agency, https://doi.org/10.5270/esa-fdsji56