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Tomographic analyses of the CMB lensing and galaxy clustering to probe the linear structure growth
Journal of Cosmology and Astroparticle Physics ( IF 6.4 ) Pub Date : 2020-05-29 , DOI: 10.1088/1475-7516/2020/05/052
Gabriela A. Marques 1, 2 , Armando Bernui 1
Affiliation  

In a tomographic approach, we measure the cross-correlation between the CMB lensing reconstructed from the Planck satellite and the galaxies of the photometric redshift catalogue based on the combination of the South Galactic Cap u-band Sky Survey (SCUSS), Sloan Digital Sky Survey (SDSS), and Wide-field Infrared Survey Explorer (WISE) data. We perform the analyses considering six redshift bins spanning the range of $0.1

中文翻译:

CMB 透镜和星系团的层析成像分析以探测线性结构增长

在断层扫描方法中,我们测量了从普朗克卫星重建的 CMB 透镜与基于南银河帽 u 波段巡天 (SCUSS)、斯隆数字巡天的组合的光度红移目录的星系之间的互相关(SDSS) 和广域红外测量探索器 (WISE) 数据。我们执行分析时考虑了跨越 0.1 美元范围的六个红移箱
更新日期:2020-05-29
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