Image Details

Choose export citation format:

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 6.

We compare our concentration and bias measurements to previous observations by I22 and S22, using different types of symbols, with average redshift of each sample within 0.2 ≤ z < 0.6. Here, we only show the results in three redshift bins, within 0.2 ≤ z < 0.5. We present the theoretical predictions under the Planck18 cosmology with the solid lines and the prediction under the cosmology obtained in I22 with the dashed lines.

Other Images in This Article
Copyright and Terms & Conditions

Additional terms of reuse