Star Formation and Nebular Attenuation from Pa alpha, Br alpha, and Br beta in Massive Dust-obscured Galaxies at Cosmic Noon using JWST

arXiv:2609.22428 · astro-ph.GA · Submitted 2026-09-18 · Read on arXiv

astro-ph.GA

Submitted: 2026-09-18

Updated: 2026-09-18

Comments: 15 pages, 10 figures

License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/

Terminology

• alpha — 2× in this paper · explained in 1 episode
• AGN — 1× in this paper · explained in 1 episode
• Active Galactic Nuclei (AGN) — 1× in this paper · explained in 1 episode
• Dust Attenuation — 1× in this paper · explained in 2 episodes
• Trace — 1× in this paper · explained in 2 episodes

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