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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 2.

The ESD of the DESI Legacy Imaging Surveys DR9 lens samples in different redshift and mass bins, as indicated, in different columns and rows. In each panel, we compare the results for three different group center indicators. The red points represent the results for the BCG group center, orange those for the LWC, and green those for the NWC. We can see that the BCG performs best as a center indicator. The solid line in each panel shows the best-fit model (Equation (7)) of the ESD for the BCG centroid. The dark and light gray shaded regions represent the 68% and 95% confidence regions of the ESD fitting results, respectively.

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