Galaxy Clusters from the DESI Legacy Imaging Surveys. II. Environmental Effects on the Size–Mass Relation
To investigate the environmental effects on the growth of galaxies, we study the size–mass relation across a broad range of environments with a vast sample of approximately 32 million galaxies at z < 0.5 from the DESI Legacy Imaging Surveys. This sample is divided into three subsamples representi...
Main Authors: | Zhaobin Chen, Yizhou Gu, Hu Zou, Qirong Yuan |
---|---|
Format: | Article |
Language: | English |
Published: |
IOP Publishing
2024-01-01
|
Series: | The Astrophysical Journal |
Subjects: | |
Online Access: | https://doi.org/10.3847/1538-4357/ad15fd |
Similar Items
-
The Emergence of a Brightest Cluster Galaxy in a Protocluster Core at z = 2.24
by: Dong Dong Shi, et al.
Published: (2024-01-01) -
Atmospheric Pressure and Molecular Cloud Formation in Early-type Galaxies
by: Iu. V. Babyk, et al.
Published: (2023-01-01) -
CLASH-VLT: The Inner Slope of the MACS J1206.2-0847 Dark Matter Density Profile
by: Andrea Biviano, et al.
Published: (2023-01-01) -
Investigating the M GCS–M h Relation in the Most Massive Galaxies
by: Veronika Dornan, et al.
Published: (2023-01-01) -
Evidence for AGN-regulated Cooling in Clusters at z ∼ 1.4: A Multiwavelength View of SPT-CL J0607-4448
by: Megan Masterson, et al.
Published: (2023-01-01)