Non-Gaussianity and direction-dependent systematics in HST Key Project data

被引:2
|
作者
Gupta, Shashikant [1 ,2 ]
Saini, Tarun Deep [2 ]
机构
[1] Raman Res Inst, Bangalore 560080, Karnataka, India
[2] Indian Inst Sci, Bangalore 560012, Karnataka, India
关键词
methods: statistical; cosmological parameters; EXTRAGALACTIC DISTANCE SCALE; HUBBLE CONSTANT; BUBBLE; SHAPES; DUST;
D O I
10.1111/j.1365-2966.2011.18882.x
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Two new statistics, namely Delta(chi 2) and Delta(chi), based on the extreme value theory, were derived by Gupta et al. We use these statistics to study the direction dependence in the HST Key Project data, which provides one of the most precise measurements of the Hubble constant. We also study the non-Gaussianity in this data set using these statistics. Our results for Delta(chi 2) show that the significance of direction-dependent systematics is restricted to well below the 1 sigma confidence limit; however, the presence of non-Gaussian features is subtle. On the other hand, the Delta(chi). statistic, which is more sensitive to direction dependence, shows direction dependence systematics to be at a slightly higher confidence level, and the presence of non-Gaussian features at a level similar to the Delta(chi 2) statistic.
引用
收藏
页码:2594 / 2599
页数:6
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