PAH emission from star-forming and quiescent galaxies at z=0.5-0.8 probed by JWST/MIRI

astro-ph.GA

Submitted: 2026-10-05

Updated: 2026-10-05

Comments: Accepted for publication in the Astrophysical Journal

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

Sources

• SMILES Initial Data Release: Unveiling the Obscured Universe with MIRI Multi-band Imaging
• Calibrating Photometric Mid-Infrared Star Formation Rates for JWST
• Overview of the JWST Advanced Deep Extragalactic Survey (JADES)
• The Galaxy Activity, Torus, and Outflow Survey (GATOS). V: Unveiling PAH survival and resilience in the circumnuclear regions of AGN with JWST
• The SMILES Mid-Infrared Survey
• AstroSat UV Deep Field South -- I. Far and Near-ultraviolet Source Catalog of the GOODS South region
• Polycyclic Aromatic Hydrocarbon Emission in the Central Regions of Three Seyferts the Implication for Underlying Feedback Mechanisms

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