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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 5.

Mass bias (Equation (26)) as a function of galaxies’ number density ngal under three different selection criterion ﹩{\nu }_{\mathrm{threshold}},{\nu }_{\mathrm{threshold}}=3.0﹩ (left), νthreshold = 4.0 (middle), and νthreshold = 5.0 (right). Large red circles show the results for the shear-selected samples, and small black circles show the results for the corresponding control samples that are selected based on noise-free νNFW instead of νobs to demonstrate that the bias is indeed caused by upscattering due to the noise. The positions of the control samples are slightly shifted rightward to avoid overlaps.

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