JWST MIRI color classification of mid-infrared selected galaxies

Context. We investigated the James Webb Space Telescope photometric color classification of mid-infrared (MIR) selected galaxies at high redshifts, toward cosmic noon. Aims. 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. Methods. 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 μm 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 ∼ 2. We applied the photometric MIR colors to the largest (∼34 arcmin 2 ) 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 ∼ 10 11.9 L ⊙ at 0.9 ≤ z < 1.57. The majority of them are consistent with the z ∼ 1 main sequence. We also identified the first examples of z ∼ 1 galaxies with deep silicate absorption.