NOEMA3D: Extended CO, [C I] and dust in massive star-forming main-sequence galaxies at cosmic noon

arXiv:2604.18504 · astro-ph.GA · Submitted 2026-04-20 · Read on arXiv

astro-ph.GA

Submitted: 2026-04-20

Updated: 2026-08-28

Code: https://github.com/1054/Crab.Toolkit.JWST

Project page: https://dawn-cph.github.io/dja/https://mast.stsci.edu/search/4https://github.com/1054/Crab.Toolkit.JWST

Terminology

• Aperture — 6× in this paper · explained in 1 episode
• Dust Attenuation — 6× in this paper · explained in 2 episodes
• AGN — 5× in this paper · explained in 1 episode
• Trace — 5× in this paper · explained in 2 episodes
• Calibration — 4× in this paper · explained in 7 episodes
• AGN Feedback — 3× in this paper · explained in 1 episode
• Core — 3× in this paper · explained in 2 episodes
• Metallicity — 3× in this paper · explained in 3 episodes
• Abundance — 2× in this paper · explained in 1 episode
• Dawn JWST Archive — 2× in this paper
• APEX — 1× in this paper · explained in 1 episode
• Active Galactic Nuclei (AGN) — 1× in this paper · explained in 1 episode
• Consistency — 1× in this paper · explained in 3 episodes
• Degeneracy — 1× in this paper · explained in 3 episodes
• Forward modeling — 1× in this paper · explained in 2 episodes
• Population Synthesis — 1× in this paper · explained in 2 episodes
• Signal-to-noise ratio (SNR) — 1× in this paper · explained in 2 episodes
• Star Formation Rate (SFR) — 1× in this paper · explained in 5 episodes

Sources

• The Great Observatories Origins Deep Survey
• NOEMA3D: Resolving radial gas flows in disk galaxies at z~1.1-1.6 with high-resolution CO observations
• NOEMA$^\rm{3D}$: A deep view of cold gas flows in a barred spiral galaxy at $z\sim1$

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