Fig. A.3.
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Comparison of the cluster ages (in Myr) as determined with different model families (PARSEC and BHAC15) and different Gaia CMDs (BPRP and GRP). We observe strong agreement between ages determined with PARSEC BPRP, PARSEC GRP, and BHAC15 GRP isochrones. In contrast, BHAC15 BPRP model fits seem to suggest systematically younger ages.
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