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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 9.

The histograms show the probability density function (pdf) of the mass bias (Equation (26)) in a 4 × 4 grid in redshift and mass. The mean of the distribution and the variance in logarithmic space are quoted in the upper left corner in each panel. In each panel, a lognormal pdf according to these two parameters is overplotted by a solid line to see how well the distribution is described by the lognormal form. These histograms are based on an ngal = 30 arcmin−2 sample selected with a νthreshold ≥ 4.0 cut. The uncertainty due to halo triaxiality is included.

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