Fig. 9
Comparison of the star formation history and cumulative stellar mass evolution between the different models of Fornax and Sextans in four cases: random IMF sampling (RIMFS), optimal IMF sampling (OIMFS), and continuous IMF sampling with an adiabatic time tad,SNIa = 5 Myr (CIMFS) and with tad,SNIa = 0 (CIMFS + tad,SNIa = 0). Each panel corresponds to a different resolution.
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