Tracing luminous infrared galaxy populations through cluster evolution in a cosmological mock redshift survey

arXiv:2608.02898 · astro-ph.GA · Submitted 2026-08-03 · Read on arXiv

Norma Araceli Nava-Moreno, Alfredo Montaña, Itziar Aretxaga, Aldo Rodríguez-Puebla, Vladimir Avila-Reese

astro-ph.GA

Submitted: 2026-08-03

Comments: 16 pages, 13 figures. Submitted to Monthly Notices of the Royal Astronomical Society

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

Terminology

• Trace — 12× in this paper · explained in 2 episodes
• Abundance — 6× in this paper · explained in 1 episode
• Gravitational Lensing — 4× in this paper · explained in 2 episodes
• Aperture — 3× in this paper · explained in 1 episode
• Benchmark — 1× in this paper · explained in 2 episodes
• Decoupling — 1× in this paper · explained in 2 episodes
• Robustness — 1× in this paper · explained in 5 episodes
• South Pole Telescope — 1× in this paper
• Ultra-Deep Survey — 1× in this paper

Sources

• The Co-Evolution Between Galaxies and Dark Matter Halos
• Too many protoclusters? Reconciling the overabundance of cluster progenitors within the first billion years of the Universe

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