The FIRST Bright Quasar Survey. III. The South Galactic cap

被引:103
|
作者
Becker, RH [1 ]
White, RL
Gregg, MD
Laurent-Muehleisen, SA
Brotherton, MS
Impey, CD
Chaffee, FH
Richards, GT
Helfand, DJ
Lacy, M
Courbin, F
Proctor, DD
机构
[1] Univ Calif Davis, Dept Phys, Davis, CA 95616 USA
[2] Lawrence Livermore Natl Lab, IGPP, Livermore, CA 94550 USA
[3] Space Telescope Sci Inst, Baltimore, MD 21218 USA
[4] Univ Arizona, Steward Observ, Tucson, AZ 85721 USA
[5] Univ Chicago, Ctr Astron & Astrophys, Chicago, IL 60637 USA
[6] Columbia Univ, Dept Astron, New York, NY 10027 USA
[7] Univ Cambridge, Inst Astron, Cambridge CB2 1TN, England
[8] Pontificia Univ Catolica Chile, Santiago de Compostela, Spain
来源
关键词
BL Lacertae objects : general; galaxies : active; galaxies : starburst; quasars : general; radio continuum : galaxies; surveys;
D O I
10.1086/321798
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present the results of an extension of the FIRST Bright Quasar Survey (FBQS) to the South Galactic cap, and to a fainter optical magnitude limit. Radio source counterparts with SERC R magnitudes brighter than 18.9 which meet the other FBQS criteria are included. We supplement this list with a modest number of additional objects to test our completeness for quasars with extended radio morphologies. The survey covers 589 deg(2) in two equatorial strips in the southern cap. We have obtained spectra for 86% of the 522 candidates and find 321 radio-selected quasars of which 264 are reported here for the first time. A comparison of this fainter sample with the FBQS sample shows the two to be generally similar. Fourteen new broad absorption line (BAL) quasars are included in this sample. When combined with the previously identified BAL quasars in our earlier papers, we can discern a break in the frequency of BAL quasars with radio loudness, namely that the relative number of high-ionization BAL quasars drops by a factor of 4 for quasars with a radio-loudness parameter R* >100.
引用
收藏
页码:227 / 262
页数:36
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