Fig. 9.

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Evolution of the bTFR zero point with redshift, shown relative to the local calibration of Lelli et al. (2019) along the stellar mass axis. Also plotted are predictions from the SIMBA hydrodynamical simulation (Glowacki et al. 2021), the Dutton et al. (2011) semi-analytical model, the empirical model of Übler et al. (2017) along with their measurements on the KMOS3D sample. Horizontal error bars indicate the redshift range of our sample while vertical error bars show the fitting uncertainties for each sample.
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