Resolved Dust in z about1 Galaxies with JWST/MIRI MRS: Survey Description and First View on PAHs, Mid-IR Atomic Emission, and Warm H 2

arXiv:2608.27560 · astro-ph.GA · Submitted 2026-08-27 · Read on arXiv

astro-ph.GA

Submitted: 2026-08-27

Updated: 2026-09-16

Terminology

• AGN — 71× in this paper · explained in 1 episode
• Dust Attenuation — 15× in this paper · explained in 2 episodes
• Aperture — 13× in this paper · explained in 1 episode
• Metallicity — 6× in this paper · explained in 3 episodes
• Abundance — 4× in this paper · explained in 1 episode
• Calibration — 2× in this paper · explained in 7 episodes
• Consistency — 2× in this paper · explained in 3 episodes
• Feature Extraction — 2× in this paper · explained in 2 episodes
• Polycyclic aromatic hydrocarbons (PAHs) — 2× in this paper · explained in 2 episodes
• Trace — 2× in this paper · explained in 2 episodes
• Active Galactic Nuclei (AGN) — 1× in this paper · explained in 1 episode
• Anti-correlation — 1× in this paper · explained in 3 episodes
• Core — 1× in this paper · explained in 2 episodes
• MIRI Medium Resolution Spectroscopy — 1× in this paper
• Monte Carlo — 1× in this paper
• Verification — 1× in this paper · explained in 2 episodes

Sources

• The ALPINE-CRISTAL-JWST Survey: The Fast Metal Enrichment of Massive Galaxies at z~5
• COSMOS Spectroscopic Redshift Compilation (First Data Release): 488k Redshifts Encompassing Two Decades of Spectroscopy
• COSMOS2025: The COSMOS-Web galaxy catalog of photometry, morphology, redshifts, and physical parameters from JWST, HST, and ground-based imaging
• Growth of Aromatic Hydrocarbon Dust Particles in the Extremely Metal-poor Galaxy Sextans A
• Aromatic Species in the Molecular Universe
• The ALPINE-CRISTAL-JWST Survey: Chemical Abundance Comparison Between the ISM and CGM of Main-Sequence Galaxies at z=4-6

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