The X-ray evolution of clusters of galaxies

被引:2
|
作者
Jones, LR [1 ]
Scharf, C
Perlman, E
Ebeling, H
Horner, D
Wegner, G
Malkan, M
McHardy, I
机构
[1] Univ Birmingham, Birmingham B15 2TT, W Midlands, England
[2] STScI, Baltimore, MD USA
[3] Univ Hawaii, Honolulu, HI 96822 USA
[4] NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA
[5] Dartmouth Coll, Hanover, NH USA
[6] Univ Calif Los Angeles, Los Angeles, CA USA
[7] Univ Southampton, Southampton, Hants, England
关键词
X-rays; clusters of galaxies;
D O I
10.1002/asna.2123190141
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The WARPS survey currently contains 48 X-ray selected clusters and groups of galaxies, detected serendipitously in ROSAT PSPC archival pointed observations. The survey includes the highest redshift X-ray selected cluster known (z=0.8325). The redshift range is large enough for evolutionary effects to be studied within the sample. Here we describe the X-ray luminosity function and Log(N)-Log(S) results for the initial complete sample of 29 spectroscopically confirmed clusters. We find that the X-ray luminosity function does not evolve at z-0.5 for cluster luminosities of similar to 10(44) erg s(-1), but that there is a hint of positive evolution at lower luminosities from the number of groups & clusters found in the faintest available X-ray cluster sample (the UK deep survey).
引用
收藏
页码:87 / 90
页数:4
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