Tomographic halo model of the unWISE-Blue galaxies using cross-correlations with BOSS CMASS galaxies
The halo model offers a framework for investigating galaxy clustering, and for understanding the growth of galaxies and the distribution of galaxies of different types. Here, we use the halo model to study the small-scale clustering and halo occupation distribution (HOD) of the unWISE-Blue galaxy sa...
Saved in:
Main Authors: | Alex Krolewski, Jensen Lawrence, Will J. Percival |
---|---|
Format: | Article |
Language: | English |
Published: |
Maynooth Academic Publishing
2025-04-01
|
Series: | The Open Journal of Astrophysics |
Online Access: | https://doi.org/10.33232/001c.137297 |
Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
Similar Items
-
The Impact of Galaxy-halo Size Relations on Galaxy Clustering Signals
by: Joshua B. Hill, et al.
Published: (2025-05-01) -
Truncations in the X-Ray Halos of Early-type Galaxies as a Tracer of Feedback and Mergers
by: Nushkia Chamba, et al.
Published: (2025-01-01) -
Predictions for the Detectability of Milky Way Satellite Galaxies and Outer-Halo Star Clusters with the Vera C. Rubin Observatory
by: Kabelo Tsiane, et al.
Published: (2025-07-01) -
Galaxies structure and evolution
by: Tayler, R. J. (Roger John)
Published: (1978) -
Stars and galaxies /
by: Kerrod, Robin
Published: (1990)