Fig. 4.

Value of Dn4000 as a function of stellar age for a set of single stellar population models from Bruzual & Charlot (2003) for different stellar metallicities from Z = 0.1 Z⊙ to Z = 2.5 Z⊙. The thick solid line shows the relation using the stellar metallicity for the median stellar mass and redshift of our sample (see Sect. 3.3). Right panel: distribution of measured Dn4000 values for the galaxies in our sample.
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