LATIS: Constraints on the Galaxy–Halo Connection at z ∼ 2.5 from Galaxy–Galaxy and Galaxy–Lyα Clustering

The connection between galaxies and dark matter halos is often quantified using the stellar mass–halo mass (SMHM) relation. Optical and near-infrared imaging surveys have led to a broadly consistent picture of the evolving SMHM relation based on measurements of galaxy abundances and angular correlat...

Full description

Saved in:
Bibliographic Details
Published in:The Astrophysical journal 2024-01, Vol.961 (1), p.27
Main Authors: Newman, Andrew B., Qezlou, Mahdi, Chartab, Nima, Rudie, Gwen C., Blanc, Guillermo A., Bird, Simeon, Benson, Andrew J., Kelson, Daniel D., Lemaux, Brian C.
Format: Article
Language:English
Subjects:
Angular correlation
Astrophysics
Autocorrelation function
Autocorrelation functions
Clustering
Correlation
Covariance matrix
Cross correlation
Dark matter
Galactic halos
Galaxies
Galaxy dark matter halos
Halos
Infrared imaging
Lyman-break galaxies
Lyα forest
Polls & surveys
Stars & galaxies
Stellar mass
Citations: Items that this one cites
Items that cite this one
Online Access:Get full text
Tags: Add Tag
No Tags, Be the first to tag this record!