Redshifts of class radio sources

被引:42
作者
Marlow, DR
Rusin, D
Jackson, N
Wilkinson, PN
Browne, IWA
Koopmans, L
机构
[1] Univ Penn, Dept Phys & Astron, Philadelphia, PA 19104 USA
[2] Univ Manchester, Nuffield Radio Astron Labs, Jodrell Bank, Macclesfield SK11 9DL, Cheshire, England
[3] Kapteyn Astron Inst, NL-9700 AV Groningen, Netherlands
关键词
gravitational lensing;
D O I
10.1086/301375
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Spectroscopic observations of a sample of 42 flat-spectrum radio sources from the Cosmic Lens All-Sky Survey (CLASS) have yielded a mean redshift of (z) = 1.27 with an rms spread of 0.95, at a completeness level of 64%. The sample consists of sources with a 5 GHz flux density of 25-50 mJy, making it the faintest flat-spectrum radio sample for which the redshift distribution has been studied. The spectra, obtained with the William Herschel Telescope, consist mainly of broad-line quasars at z > 1 and narrow-line galaxies at z < 0.5. Though the mean redshift of flat-spectrum radio sources exhibits little variation over more than 2 orders of magnitude in radio flux density, there is evidence of a decreasing fraction of quasars at weaker flux levels. We present the results of our spectroscopic observations and discuss the implications for constraining cosmological parameters with statistical analyses of CLASS.
引用
收藏
页码:2629 / 2633
页数:5
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