Dissect two-halo galactic conformity effect for central galaxies: The dependence of star formation activities on the large-scale environment

arXiv:2304.06886 · astro-ph.GA, astro-ph.CO · Submitted 2023-07-21 · Read on arXiv

Kai Wang, Yingjie Peng, Yangyao Chen

astro-ph.GA, astro-ph.CO

Submitted: 2023-07-21

Updated: 2026-08-19

Comments: 13 pages, 9 figures, MNRAS 523 1268

Journal ref: MNRAS, Volume 523, Issue 1, July 2023, Pages 1268-1279

DOI: 10.1093/mnras/stad1169

Code: https://github.com/ChenYangyao/hipp

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

Terminology

• Velocity Dispersion — 6× in this paper · explained in 2 episodes
• AGN — 4× in this paper · explained in 1 episode
• AGN Feedback — 2× in this paper · explained in 1 episode
• Abundance — 2× in this paper · explained in 1 episode
• Aperture — 2× in this paper · explained in 1 episode
• Adam — 1× in this paper · explained in 2 episodes
• Calibration — 1× in this paper · explained in 7 episodes
• Clustering — 1× in this paper · explained in 2 episodes
• Galaxy Quenching — 1× in this paper · explained in 3 episodes
• Robustness — 1× in this paper · explained in 5 episodes
• Star Formation Rate (SFR) — 1× in this paper · explained in 5 episodes
• Weak Lensing — 1× in this paper · explained in 2 episodes

Sources

• Late-formed halos prefer to host quiescent central galaxies. I. Observational results

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