Intracluster light as a dark matter tracer: how their spatial and kinematic relationship is shaped by satellite demographics

arXiv:2601.18693 · astro-ph.GA, astro-ph.CO · Submitted 2026-01-26 · Read on arXiv

astro-ph.GA, astro-ph.CO

Submitted: 2026-01-26

Updated: 2026-08-28

Comments: Updated author metadata

DOI: 10.1093/mnras/stag649

Code: https://github.com/garrethmartin/bh_

Project page: https://www.horizon-simulation.org

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

Terminology

AGN — 24× in this paper · explained in 1 episode
Abundance — 7× in this paper · explained in 1 episode
Trace — 7× in this paper · explained in 2 episodes
AGN Feedback — 4× in this paper · explained in 1 episode
Stellar Feedback — 3× in this paper · explained in 2 episodes
Weak Lensing — 3× in this paper · explained in 2 episodes
Adiabatic Evolution — 2× in this paper · explained in 2 episodes
Alignment — 1× in this paper · explained in 1 episode
Angular Momentum Loss — 1× in this paper · explained in 1 episode
Bayesian Inference — 1× in this paper · explained in 5 episodes
Consistency — 1× in this paper · explained in 3 episodes
Degeneracy — 1× in this paper · explained in 3 episodes
Gauss Centre for Supercomputing — 1× in this paper
Markov Chain Monte Carlo — 1× in this paper
N-body simulations — 1× in this paper · explained in 2 episodes
Robustness — 1× in this paper · explained in 5 episodes

Sources

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