Integrated Sachs-Wolfe effect map recovery from NVSS and WMAP 7-yr data

被引:11
作者
Barreiro, R. B. [1 ]
Vielva, P. [1 ]
Marcos-Caballero, A. [1 ,2 ]
Martinez-Gonzalez, E. [1 ]
机构
[1] Univ Cantabria, CSIC, Inst Fis Cantabria, E-39005 Santander, Spain
[2] Univ Cantabria, Dept Fis Moderna, E-39005 Santander, Spain
关键词
methods: data analysis; methods: statistical; cosmology: observations; cosmic background radiation; large-scale structure of Universe; LARGE-SCALE STRUCTURE; COSMOLOGICAL CONSTANT; POWER SPECTRUM; DARK ENERGY; MICROWAVE; RADIO; ESTIMATOR; SIGNAL; ISW; CMB;
D O I
10.1093/mnras/sts600
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present a map of the cosmic microwave background (CMB) anisotropies induced by the late integrated Sachs-Wolfe effect. The map is constructed by combining the information of the Wilkinson Microwave Anisotropy Probe 7-yr CMB data and the NRAO VLA Sky Survey (NVSS) through a linear filter. This combination improves the quality of the map that would be obtained using information only from the large-scale structure data. In order to apply the filter, a given cosmological model needs to be assumed. In particular, we consider the standard Lambda cold dark matter model. As a test of consistency, we show that the reconstructed map is in agreement with the assumed model, which is also favoured against a scenario where no correlation between the CMB and NVSS catalogue is considered.
引用
收藏
页码:259 / 263
页数:5
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