Statistical evaluation of the observational information on Ωm and ΩΛ

被引:7
作者
Harun-or-Rashid, SM [1 ]
Roos, M [1 ]
机构
[1] Univ Helsinki, Dept Phys, Div High Energy Phys, FIN-00014 Helsinki, Finland
来源
ASTRONOMY & ASTROPHYSICS | 2001年 / 373卷 / 02期
关键词
cosmology : observations; methods : statistical;
D O I
10.1051/0004-6361:20010627
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We undertake a critical evaluation of recent observational information on Omega (m) and Omega (Lambda) in order to identify possible sources of systematic errors and effects of simplified statistical analyses. We combine observations for which the results have been published in the form of likelihood contours in the Omega (m), Omega (Lambda) plane. We approximate the contours by fifth order polynomials, and we then use the maximum likelihood method to obtain joint likelihood contours for the combined data. In the choice of statistical merits we aim at minimum loss of information rather than at minimum variance. We find that Omega (0) = Omega (m) + Omega (Lambda) = 0.99 +/- 0.04 +/- 0.03, where the first error is mainly statistical and the second error is systematical. In a at Universe we find Omega (flat)(m) = 0.31 +/- 0.04 +/- 0.04.
引用
收藏
页码:369 / 376
页数:8
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