Fig. 4.
Clusters for which an eMSTO has been observed in the LMC (from Goudfrooij et al. 2014, 2017; Milone et al. 2015, 2017, 2018; Niederhofer et al. 2015b; Bastian et al. 2016; Martocchia et al. 2018, filled circles) and in the Galaxy (Bastian et al. 2018; Cordoni et al. 2018, open circles). Down arrows correspond to upper limits. Coloured curves are the results in term of equivalent age spread from our simulations at three metallicities for both stellar evolution codes (see text for full description of line types).
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