A comparison of estimators for the two-point correlation function

被引:173
作者
Kerscher, M [1 ]
Szapudi, I
Szalay, AS
机构
[1] Johns Hopkins Univ, Dept Phys & Astron, Baltimore, MD 21218 USA
[2] Univ Munich, D-80333 Munich, Germany
[3] Univ Toronto, Canadian Inst Theoret Astrophys, Toronto, ON M5S 3H8, Canada
基金
美国国家科学基金会;
关键词
galaxies : clusters : general; methods : statistical;
D O I
10.1086/312702
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Nine of the most important estimators known for the two-point correlation function are compared using a predetermined, rigorous criterion. The indicators were extracted from over 500 subsamples of the Virgo Hubble volume simulation cluster catalog. The "real" correlation function was determined from the full survey in a 3000 h(-1) Mpc periodic cube, The estimators were ranked by the cumulative probability of returning a value within a certain tolerance of the real correlation function. This criterion takes into account bias and variance, and it is independent of the possibly non-Gaussian nature of the error statistics. As a result, for astrophysical applications, a clear recommendation has emerged: the Landy & Szalay estimator, in its original or grid version (Szapudi & Szalay), is preferred in comparison with the other indicators examined, with a performance almost indistinguishable from the Hamilton estimator.
引用
收藏
页码:L13 / L16
页数:4
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