Fig. A.4.
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Slopes of the SF gradients as a function of the stellar mass. For a comparison to other works, see the shape of the relation derived by Mingozzi et al. (2020) using the code IZI (Blanc et al. 2014) coupled with MAPPINGS IV photoionization models (e.g., red line in the right panel from Figure 12 of the paper) and by Franchetto et al. (2020) using the PYQZ code (Dopita et al. 2013) coupled with the same models as in Mingozzi et al. (2020).
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