A dataset provided by the European Space Agency

Name 9045
Title The Relationship Between Radio Luminosity and Radio-Loud AGN Host Galaxy Properties
URL https://hst.esac.esa.int/ehst/#/pages/search;proposal=9045;TAPCLIENT=DOI
DOI https://doi.org/10.5270/esa-oixpeel
Author Willott, Chris J.
Description This is a scientific proposal for HST mission. For specific information please visit https://archive.stsci.edu/proposal_search.php?id=9045&mission=hst
Publication
  • A sample of radio galaxies spanning three decades in radio luminosity - I. The host galaxy properties and black hole masses
  • Merger-driven Growth of Intermediate-mass Black Holes: Constraints from Hubble Space Telescope Imaging of Hyper-luminous X-Ray Sources
  • Molecular gas in distant brightest cluster galaxies
  • Radio galaxy host properties spanning three dex in radio luminosity
  • Radio Loud AGNs are Mergers
  • The nuclear radio-optical properties of intermediate-redshift FR II radio galaxies and quasars
  • The Origins of X-Ray Emission from the Hot Spots of FR II Radio Sources
Instrument WFPC2, WFPC2/PC
Temporal Coverage 2001-05-21T00:57:14Z/2001-11-28T23:20:35Z
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 2002-11-29T01:00:46Z
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, Willott comma Chris J., 2002, 'The Relationship Between Radio Luminosity and Radio-Loud AGN Host Galaxy Properties', 1.0, European Space Agency, https://doi.org/10.5270/esa-oixpeel