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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 3.

The best-fit results and different model components for a lens sample with mass ﹩14.0\leqslant \mathrm{log}{M}_{{\rm{G}}}\lt 14.4﹩ at redshift 0.3 ≤ z < 0.4. The dark and light gray shaded regions represent the 68% and 95% confidence intervals of the total ESD fitting results, respectively. The three panels correspond to the three different types of group center. The different colored lines represent the halo components labeled in the legend. The χ 2/ν value is also provided in each panel. Note that the degrees of freedom have a value of ν = 15 here.

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