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18 April 2024 |
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The FIRST Bright QSO Survey | Michael D. Gregg
; Robert H. Becker
; Richard L. White
; David J. Helfand
; Richard G. McMahon
; Isobel M. Hook
; | Date: |
25 Apr 1996 | Subject: | astro-ph | Affiliation: | IGPP/LLNL), Robert H. Becker (UC Davis), Richard L. White (STScI), David J. Helfand (Columbia), Richard G. McMahon (Cambridge), Isobel M. Hook (UC Berkeley | Abstract: | The FIRST Radio Survey provides a new resource for constructing a large quasar sample. With source positions accurate to better than 1arcsec 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$^2$ 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 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 E magnitude of 14.6 and z = 0.91; four others are brighter than E = 16. The redshifts range from z=0.12 to 3.42. Half of the detected objects are radio quiet with L$_{
m 21cm} < 10^{32.5}$ 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 70efficient and 95complete to a 21-cm flux density limit of 1.0 mJy. | Source: | arXiv, astro-ph/9604148 | Services: | Forum | Review | PDF | Favorites |
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