Fig. 10.

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Lower panel: Our fit of the SFMS, in the four redshift bins (stars with error bars and arrows) and best-fit model (dashed lines). The reported redshift is the median z of the bin. Upper panels: Best-fit (red stars) and reported (squares for Popesso et al. 2023; circles for Daddi et al. 2022a) values for the bending mass and maximum SFR, defined as ℳ0 ≡ log10(M0/M⊙) and 𝒮ℱℛmax ≡ log10(SFRmax/M⊙ yr−1), as a function of redshift.
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