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Analysis of the clustering of 2dFGRS galaxies using the method of a modibed correlation gamma function

机译:使用改进的相关伽马函数方法分析2dFGRS星系的聚类

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The apparatus of a correlation gamma function is used to analyze a sample of 2dFGRS galaxies. We suggest a modified gamma-function algorithm with nonintersecting working spheres, which ensures that the counts are independent at each step. The method of nonintersecting spheres has revealed a change in the regime of clustering (a break of the gamma function) on a scale of 10-16h(-1) Mpc (H-0 = 65 km s(-1) Mpc(-1)). The standard method yields a scale of 30h(-1) Mpc. An artificial distribution is used as an example to show that, in some cases, the modified algorithm is more responsive to a mixture of distributions with various properties than the standard method. (c) 2005 Pleiades Publishing, Inc.
机译:相关伽马函数的设备用于分析2dFGRS星系的样本。我们建议使用不相交的工作范围的改进的伽马函数算法,以确保计数在每个步骤都是独立的。非相交球体的方法揭示了聚类状态的变化(伽马函数的破坏),变化范围为10-16h(-1)Mpc(H-0 = 65 km s(-1)Mpc(-1 ))。标准方法的规模为30h(-1)Mpc。以人工分布为例来说明,在某些情况下,与标准方法相比,修改后的算法对具有各种属性的分布混合更敏感。 (c)2005年Pleiades Publishing,Inc.

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