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Mass Bias of Weak-lensing Shear-selected Galaxy Cluster Samples

  • Authors: Kai-Feng Chen, Masamune Oguri, Yen-Ting Lin, and Satoshi Miyazaki

2020 The Astrophysical Journal 891 139.

  • Provider: AAS Journals

Caption: Figure 10.

Reconstruction of input mass function from the observed number counts of shear-selected clusters selected in an ngal = 30 arcmin−2 sample with a νthreshold ≥ 4.0 cut. The dotted histograms show the observed number density of clusters in this sample, and the reconstructed mass functions are shown in error bars. The true number density in each bin based on the input mass function from Tinker et al. (2008) is plotted as the solid histogram.

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