MUSE-ALMA Haloes XVI: a census of the condensed baryons in z 0.5 HI absorption-selected galaxies

arXiv:2610.10117 · astro-ph.GA · Submitted 2026-10-07 · Read on arXiv

astro-ph.GA

Submitted: 2026-10-07

Updated: 2026-10-07

Terminology

• Velocity Dispersion — 14× in this paper · explained in 2 episodes
• Metallicity — 12× in this paper · explained in 3 episodes
• Trace — 6× in this paper · explained in 2 episodes
• Aperture — 3× in this paper · explained in 1 episode
• Consistency — 3× in this paper · explained in 3 episodes
• AGN — 2× in this paper · explained in 1 episode
• Calibration — 2× in this paper · explained in 7 episodes
• European Research Council — 2× in this paper
• MUSE Python Data Analysis Framework — 2× in this paper
• Accuracy — 1× in this paper · explained in 1 episode
• Active Galactic Nuclei (AGN) — 1× in this paper · explained in 1 episode
• Adam — 1× in this paper · explained in 2 episodes
• Baryonic Feedback — 1× in this paper · explained in 3 episodes
• Benchmark — 1× in this paper · explained in 2 episodes
• Benchmarking — 1× in this paper · explained in 3 episodes
• Degeneracy — 1× in this paper · explained in 3 episodes
• Initial Mass Function (IMF) — 1× in this paper · explained in 2 episodes
• Star Formation Rate (SFR) — 1× in this paper · explained in 5 episodes

Sources

• MUSE-ALMA Haloes XIII. Molecular gas in $z \sim 0.5$ HI-selected galaxies
• CHILES X: Molecular and atomic gas at intermediate redshift
• Kennicutt-Schmidt relation of galaxies over 13 billion years in the COLIBRE hydrodynamical simulations
• The Multi-Scale Multi-Phase Circumgalactic Medium: Observed and Simulated
• The COLIBRE project: cosmological hydrodynamical simulations of galaxy formation and evolution
• FEASTS and MHONGOOSE: HI Column Density Distribution at $z=0$ for $N_\mathrm{HI}>10^{17.8}\, \mathrm{cm}^{-2}$

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