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Models derived in 2009 to fit mid-infrared (8-24 micron) source counts fromthe IRAS, ISO and Spitzer missions, provide an excellent fit to deep countswith JWST, demonstrating that the evolution of dusty star-forming galaxies iswell understood. The evolution of dust in galaxies at high redshifts isdiscussed and a simple prescription is proposed to model this. This allows morerealistic models for source-counts at submillimetre wavelength. A reasonablefit to 250, 500, 850 and 1100 micron counts is obtained. This paper thereforedraws together the IRAS, ISO, Spitzer, Akari, Herschel, submillimetreground-based, and JWST surveys into a single picture.

Modelling JWST mid-infrared counts: excellent consistency with models derived for IRAS, ISO and Spitzer