Fig. 3
Slopes of the non-normalized (upper panel) and normalized (lower panel) metallicity gradients of the SPs in the disc components as a function of total stellar mass of the simulated galaxies (solid, blue circles). The error bars correspond to a bootstrap error of the linear regression fits. Observations from the CALIFA survey by (Sánchez-Blázquez et al. 2014; open yellow squares) were included for comparison.
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