The connection between massive galaxies and their dark matter haloes from z=0.25 to z about 4 from the combined COSMOS, XMM-LSS and ECDF-S fields

astro-ph.GA, astro-ph.CO

Submitted: 2026-10-13

Updated: 2026-10-13

Comments: 28 pages, 18 figures, 3 tables, Accepted for publication in MNRAS

Code: https://github.com/rmjarvis/TreeCorr

License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/

Sources

• The MeerKAT International GHz Tiered Extragalactic Exploration (MIGHTEE) Survey
• Tracing the galaxy-halo connection with galaxy clustering in COSMOS-Web from z = 0.1 to z ~ 12
• COSMOS-Web: does halo mass alone shape the clustering of star-forming and quiescent galaxies?
• The VOICE Survey : VST Optical Imaging of the CDFS and ES1 Fields
• The FENIKS Survey: Stellar-Halo Mass Relationship of Central and Satellite Galaxies in UDS and COSMOS at 0.2 < z < 4.5

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