The ALHAMBRA survey: Estimation of the clustering signal encoded in the cosmic variance
Aims: The relative cosmic variance (σv) is a fundamental source of uncertainty in pencil-beam surveys and, as a particular case of count-in-cell statistics, can be used to estimate the bias between galaxies and their underlying dark-matter distribution. Our goal is to test the significance of the clustering information encoded in the σv measured in
López-Sanjuan, C. et al.
Advertised on:
10
2015