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The FIRST bright QSO survey

Journal Article · · Astronomical Journal
DOI:https://doi.org/10.1086/118024· OSTI ID:286297
 [1];  [2];  [3];  [4];  [5];  [6]
  1. Institute for Geophysics and Planetary Physics, Lawrence Livermore National Laboratory, Livermore, California 94550 (United States)
  2. University of California at Davis, Davis, California 95616 (United States)
  3. Space Telescope Science Institute, Baltimore, Maryland 21218 (United States)
  4. Columbia Astrophysics Laboratory, Columbia University, New York, New York 10027 (United States)
  5. Institute of Astronomy, Cambridge CB3 0HA (England)
  6. University of California at Berkeley, Berkeley, California 94720 (United States)
The FIRST radio survey provides a new resource for constructing a large quasar sample. With source positions accurate to better than 1{double_prime} and a point source sensitivity limit of 1 mJy, it reaches 50 times deeper than previous radio catalogs. We report here on the results of the pilot phase for a FIRST Bright Quasar Survey (FBQS). Based on matching the radio catalog from the initial 300 deg{sup 2} of FIRST coverage with the optical catalog from the Automated Plate Machine (APM) digitization of Palomar Sky Survey plates, we have defined a sample of 219 quasar candidates brighter than {ital E} = 17.50. We have obtained optical spectroscopy for 151 of these and classified 25 others from the literature, yielding 69 quasars or Seyfert 1 galaxies, of which 51 are new identifications. The brightest new quasar has an {ital E} magnitude of 14.6 and {ital z} = 0.91; four others are brighter than {ital E} = 16. The redshifts range from {ital z} = 0.12 to 3.42. Half of the detected objects are radio quiet with {ital L}{sub 21-cm}{lt}10{sup 32.5} ergs/s. We use the results of this pilot survey to establish criteria for the FBQS that will produce a quasar search program which will be 70{percent} efficient and 95{percent} complete to a 21-cm flux density limit of 1.0 mJy. {copyright} {ital 1996 American Astronomical Society.}
Research Organization:
Lawrence Livermore National Laboratory
DOE Contract Number:
W-7405-ENG-48
OSTI ID:
286297
Journal Information:
Astronomical Journal, Journal Name: Astronomical Journal Journal Issue: 2 Vol. 112; ISSN ANJOAA; ISSN 0004-6256
Country of Publication:
United States
Language:
English

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