A dataset provided by the European Space Agency

Name 10717
Title Quasar Bolometri Luminosity and Spectral Energy Distributions from Radio to X-ray
URL https://hst.esac.esa.int/ehst/#/pages/search;proposal=10717;TAPCLIENT=DOI
DOI https://doi.org/10.5270/esa-cs0rcoj
Author Shang, Zhaohui
Description This is a scientific proposal for HST mission. For specific information please visit https://archive.stsci.edu/proposal_search.php?id=10717&mission=hst
Publication
  • Comparison of the active galactic nuclei Baldwin effect with the modified Baldwin effect of the ultraviolet-optical emission lines in a single sample
  • Rehabilitating C IV-based black hole mass estimates in quasars
  • The behaviour of quasar C IV emission-line properties with orientation
  • The far-infrared emitting region in local galaxies and QSOs: Size and scaling relations
  • The Next Generation Atlas of Quasar Spectral Energy Distributions from Radio to X-Rays
  • The Optical and Ultraviolet Emission-line Properties of Bright Quasars with Detailed Spectral Energy Distributions
  • The orientation dependence of quasar single-epoch black hole mass scaling relationships
  • The orientation dependence of quasar spectral energy distributions
  • Updating quasar bolometric luminosity corrections
Instrument NICMOS, NICMOS/NIC2
Temporal Coverage 2005-10-29T00:21:40Z/2006-03-18T04:21:23Z
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 2007-03-18T14:04:27Z
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, Shang et al., 2007, 'Quasar Bolometri Luminosity and Spectral Energy Distributions from Radio to X-ray', 1.0, European Space Agency, https://doi.org/10.5270/esa-cs0rcoj