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Halo Properties and Mass Functions of Groups/Clusters from the DESI Legacy Imaging Surveys DR9

  • Authors: Jiaqi Wang, Xiaohu Yang, Jun Zhang, Hekun Li, Matthew Fong, Haojie Xu, Min He, Yizhou Gu, Wentao Luo, Fuyu Dong, Yirong Wang, Qingyang Li, Antonios Katsianis, Haoran Wang, Zhi Shen, Pedro Alonso Vaquero, Cong Liu, Yiqi Huang, Zhenjie Liu

Jiaqi Wang et al 2022 The Astrophysical Journal 936 .

  • Provider: AAS Journals

Caption: Figure 4.

An example of the marginalized posterior distributions of the five parameters ﹩\mathrm{log}{M}_{{\rm{h}}}﹩, R sig, f cen, c, and b h for the lens sample with mass ﹩14.0\leqslant \mathrm{log}{M}_{{\rm{G}}}\lt 14.4﹩ at redshift 0.3 ≤ z < 0.4. Here, the red, orange, and green contours show the results for BCG, LWC, and NWC centroids, respectively. The solid red lines show the best-fit results for the BCG sample. The dashed red lines show the 1σ confidence intervals.

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