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2025MNRAS.539.3714R - Mon. Not. R. Astron. Soc., 539, 3714-3721 (2025/June-1)

Modelling JWST mid-infrared counts - II. Extension to 5.6 μm, optical, radio, and X-rays.

ROWAN-ROBINSON M.

Abstract (from CDS):

In Paper I, models derived in 2009 to fit mid-infrared (8-24 micron) source counts from the IRAS, ISO, and Spitzer missions, were found to provide an excellent fit to deep counts at 7.7-21 $\mu$m with JWST, demonstrating that the evolution of dusty star-forming galaxies is well understood. Here, the treatment of optical spectral energy distributions is improved and the counts are extended to 5.6 $\mu$m and optical wavelengths. The models proved a good fit to the latest, deeper, JWST counts. The models are also extended to radio and X-ray wavelengths. Predicted redshift distributions are given for a range of wavelengths and flux-densities.

Abstract Copyright: © 2025 The Author(s). Published by Oxford University Press on behalf of Royal Astronomical Society.

Journal keyword(s): stars: formation - galaxies: evolution - galaxies: starburst - cosmology: observations - infrared: galaxies

Simbad objects: 3

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