Comparison between the fractions of early and late-type galaxies (top row) and disturbed and undisturbed galaxies (bottom row) as a function of stellar mass measured in CANDELS (dashed lines) and CEERS (sold lines) for exactly the same galaxies. For CANDELS, the morphologies are inferred in the F160W filter while for CEERS we use F150W in all panels to reduce wavelength induced differences in the morphologies. Each panel indicates a redshift bin as labeled.