Multi-tracer exploration of molecular gas in main sequence galaxies at z 4.5

arXiv:2609.03166 · astro-ph.GA · Submitted 2026-09-02 · Read on arXiv

astro-ph.GA

Submitted: 2026-09-02

Updated: 2026-09-02

Terminology

• Metallicity — 36× in this paper · explained in 3 episodes
• Calibration — 11× in this paper · explained in 7 episodes
• Trace — 11× in this paper · explained in 2 episodes
• Abundance — 4× in this paper · explained in 1 episode
• AGN — 3× in this paper · explained in 1 episode
• Accuracy — 2× in this paper · explained in 1 episode
• Consistency — 2× in this paper · explained in 3 episodes
• Anti-correlation — 1× in this paper · explained in 3 episodes
• Benchmark — 1× in this paper · explained in 2 episodes
• Cooperation — 1× in this paper · explained in 2 episodes
• Dust Attenuation — 1× in this paper · explained in 2 episodes
• Velocity Dispersion — 1× in this paper · explained in 2 episodes

Sources

• Cosmic evolution of the [CII]-to-molecular gas relation
• Stellar feedback SPICEs up [C II] emission in the first galaxies
• The ALMA-CRISTAL survey: Resolved kinematic studies of main sequence star-forming galaxies at 4<z<6
• The ALPINE-CRISTAL-JWST Survey: Stellar and nebular dust attenuation of main-sequence galaxies at z~4-6

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