TRICEPS. I. Tracing cold gas, dust, and stars at sub-kpc scales in massive star-forming galaxies at z = 4-5

arXiv:2609.30375 · astro-ph.GA, astro-ph.CO · Submitted 2026-09-24 · Read on arXiv

astro-ph.GA, astro-ph.CO

Submitted: 2026-09-24

Updated: 2026-09-24

Terminology

• AGN — 7× in this paper · explained in 1 episode
• Aperture — 4× in this paper · explained in 1 episode
• Trace — 3× in this paper · explained in 2 episodes
• Velocity Dispersion — 3× in this paper · explained in 2 episodes
• AGN Feedback — 2× in this paper · explained in 1 episode
• Atacama Large Millimeter Array — 1× in this paper
• Calibration — 1× in this paper · explained in 7 episodes
• Common Astronomy Software Applications — 1× in this paper
• Cooperation — 1× in this paper · explained in 2 episodes
• Degeneracy — 1× in this paper · explained in 3 episodes
• Signal-to-noise ratio (SNR) — 1× in this paper · explained in 2 episodes
• alpha — 1× in this paper · explained in 1 episode

Sources

• Dynamical Characterization of Galaxies at z~4-6 via Tilted Ring Fitting to ALMA [CII] Observations
• Charting the main sequence of star-forming galaxies out to redshifts z<5.7
• A hidden active galactic nucleus powering bright [O III] nebulae in a protocluster at $z=4.5$ revealed by JWST
• CASA, the Common Astronomy Software Applications for Radio Astronomy

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