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arXiv · 2512.16589

JWST MIRI color classification of mid-infrared selected galaxies: MIRI color classification toward cosmic noon

Ece Kilerci·Tomotsugu Goto·Matthew A. Malkan·Seong Jin Kim·Chih-Teng Ling·Cossas C. -K Wu·Tetsuya Hashimoto·Simon C. -C. Ho·Amos Y. -A. Chen·Ersin Gogus
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Abstract

We investigated the James Webb Space Telescope photometric color classification of mid-infrared (MIR) selected galaxies at high redshifts, toward cosmic noon. The aim of the present work is to obtain a z-dependent mid-infrared (MIR) photometric galaxy classification tool based on broad spectral emission and absorption lines using the JWST Mid-Infrared Instrument (MIRI) and its broadband filters. We used the largest Spitzer MIR spectral database to obtain synthetic photometry in the JWST/MIRI filters. We formed MIRI filter combinations to trace the strong polycyclic aromatic hydrocarbon (PAH) emission features and the 9.7 micron silicate feature in seven redshift windows from z = 0.25-2.10. Results. We present z-dependent MIRI color-color plots that separate active galactic nuclei (AGN), star-forming galaxies (SFGs), and silicate absorption-dominated galaxies up to z$\sim$2. We applied the photometric MIR colors to the largest ($\sim$34 arcmin square) MIRI survey called the Systematic Mid-infrared Instrument Legacy Extragalactic Survey (SMILES), to identify AGN, SFGs, and Si-absorption dominated galaxies out to substantial redshifts. Our JWST/MIRI SFGs sample includes galaxies with total IR luminosities of $10^{9.2} \sim 10^{11.9} L_{\odot}$ at 0.9 $\leq$z < 1.57. The majority of them are consistent with the z$\sim$1 main sequence. We also identified the first examples of z$\sim$1 galaxies with deep silicate absorption.

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Ece Kilerci, Tomotsugu Goto, Matthew A. Malkan, Seong Jin Kim, Chih-Teng Ling, Cossas C. -K Wu, Tetsuya Hashimoto, Simon C. -C. Ho, Amos Y. -A. Chen, Ersin Gogus. 2025-12-18. JWST MIRI color classification of mid-infrared selected galaxies: MIRI color classification toward cosmic noon. https://doi.org/10.1051/0004-6361%2F202554884

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