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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 8.

Mass bias (Equation (26)) as a function of the selection criterion νthreshold. The large red circles show the sample constructed in Section 2.1, whereas the green triangles represent the sample including the modification of halo triaxiality from Section 2.2. The dotted green line shows a quantitative estimate of the results with halo triaxiality (see Section 3.2 for details). The large red circles and the small black circles are slightly shifted leftward and rightward, respectively, from the green triangles to avoid overlaps.

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