Fig. 10.
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sSFR distribution in different stellar mass bins at redshift two, for various cosmological simulations (TNG100, SIMBA, and EAGLE) and the observational JWST/NIRCam data (derived with EAZY). The vertical orange line in the highest-mass bin marks our threshold to select massive, star-forming galaxies in TNG100. Galaxies with a sSFR below the shown log10(sSFR) grid are assigned to the lowest sSFR bin. The galaxy main sequence in the cosmological simulations diverges at high stellar masses, but they all exhibit a population of massive, star-forming galaxies as seen in the observations.
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