Fig. D.1.
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Age–metallicity relation of the mass transformed into stars as a function of time and [M/H] derived from three mother CMDs with different numbers of stars down to MG = 5, calculated from the BaSTI stellar evolution library adopting qmin = 0.1, β = 0.3, and a Kroupa IMF. They are the mother CMDs named q01b03_60M_deep, q01b03_112M_MG6, and q01b03_120M_MG5 in Table 2.
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