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Fig. 1.


From top to bottom: mass-weighted age, formation epoch, metallicity, and extinction of quiescent galaxies using EMILES+Padova00 models plotted on the circularised radius vs. stellar mass plane down to z = 0.9. All values are colour-coded as indicated by each colour bar and averaged with the LOESS method (for more details, see Sect. 3). The dashed line illustrates the median circularised radius. The number of galaxies in each panel is pointed out in the first row.

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