The galactic HI-to-halo mass relation from isolated galaxies to cosmological hydrodynamic simulations

arXiv:2609.27111 · astro-ph.GA · Submitted 2026-09-22 · Read on arXiv

astro-ph.GA

Submitted: 2026-09-22

Updated: 2026-09-22

Code: https://github.com/syrte/ndtest

Terminology

Abundance — 6× in this paper · explained in 1 episode
Trace — 4× in this paper · explained in 2 episodes
AGN — 3× in this paper · explained in 1 episode
Core — 2× in this paper · explained in 2 episodes
Spitzer Photometry and Accurate Rotation Curves — 2× in this paper
AGN Feedback — 1× in this paper · explained in 1 episode
Center for Astrophysics and Space Science — 1× in this paper
Clustering — 1× in this paper · explained in 2 episodes
Consistency — 1× in this paper · explained in 3 episodes
European Regional Development Fund — 1× in this paper
Giant Metrewave Radio Telescope — 1× in this paper
Markov Chain Monte Carlo — 1× in this paper
Robustness — 1× in this paper · explained in 5 episodes
Wide-field Infrared Survey Explorer — 1× in this paper

Sources

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