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The discovery of an X-ray selected, radio-loud quasar at z = 3. 9

Journal Article · · Astronomical Journal; (United States)
DOI:https://doi.org/10.1086/116251· OSTI ID:7159137
; ;  [1]
  1. California, University, Davis (United States) Lawrence Livermore National Laboratory, Livermore, CA (United States) Columbia University, NY (United States) Joint Institute for Laboratory Astrophysics, Boulder, CO (United States) Space Telescope Science Institute, Baltimore, MD (United States)
About 600 weak X-ray sources from a data base of about 100,000 2-4sigma fluctuations derived from Einstein Observatory imaging proportional counter X-ray images are selected on the basis of a flux-limited catalog of radio sources in the northern sky. Optical spectroscopy of only six of these sources resulted in the discovery of a quasar with an emission-line redshift of 3.87. Subsequent VLA observations reveal the source to have a flat-spectrum radio core plus an unresolved radio lobe 2.5 arcsec away with a spectral index of 1.45. The lobe is connected to the core by a weak jet. The integrated flux density of the source at 20 cm is 0.66 Jy. The v magnitude of the quasar is 19.5, and the tentative X-ray sources has a very soft spectrum. The properties of this object are discussed in the context of known high-redshift radio sources and existing X-ray selected quasar samples, and the potential of the present discovery technique for examining the properties of very distant active galaxies is explored. 20 refs.
OSTI ID:
7159137
Journal Information:
Astronomical Journal; (United States), Journal Name: Astronomical Journal; (United States) Vol. 104:2; ISSN ANJOAA; ISSN 0004-6256
Country of Publication:
United States
Language:
English