Constraints on cosmological parameters from the analysis of the Cosmic Lens All Sky Survey radio-selected gravitational lens statistics

被引:116
作者
Chae, KH [1 ]
Biggs, AD
Blandford, RD
Browne, IWA
de Bruyn, AG
Fassnacht, CD
Helbig, P
Jackson, NJ
King, LJ
Koopmans, LVE
Mao, S
Marlow, DR
McKean, JP
Myers, ST
Norbury, M
Pearson, TJ
Phillips, PM
Readhead, ACS
Rusin, D
Sykes, CM
Wilkinson, PN
Xanthopoulos, E
York, T
机构
[1] Univ Manchester, Jodrell Bank Observ, Macclesfield SK11 9DL, Cheshire, England
[2] CALTECH, Pasadena, CA 91125 USA
[3] Netherlands Fdn Res Astron, NL-7990 AA Dwingeloo, Netherlands
[4] Space Telescope Sci Inst, Baltimore, MD 21218 USA
[5] Univ Bonn, D-53121 Bonn, Germany
[6] Univ Penn, Dept Phys & Astron, Philadelphia, PA 19104 USA
[7] Natl Radio Astron Observ, Socorro, NM 87801 USA
[8] Harvard Smithsonian Ctr Astrophys, Cambridge, MA 02138 USA
关键词
D O I
10.1103/PhysRevLett.89.151301
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
We derive constraints on cosmological parameters and the properties of the lensing galaxies from gravitational lens statistics based on the final Cosmic Lens All Sky Survey data. For a flat universe with a classical cosmological constant, we find that the present matter fraction of the critical density is Omega(m)=0.31(-0.14)(+0.27) (68%)(-0.10)(+0.12) (syst). For a flat universe with a constant equation of state for dark energy w=p(x)(pressure)/rho(x)(energy density), we find w<-0.55(-0.11)(+0.18) (68%).
引用
收藏
页码:151301/1 / 151301/4
页数:4
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