Evolution stage distribution from FLAME in the CMDs of some selected clusters. The top panels represent the CMDs of four open clusters near solar metallicity, and the bottom panels are those of four low-metallicity globular clusters. Gaia Collaboration (2018b) provided the cluster members. We parsed the values of astrophysical_parameters.evolstage_flame into the three stages: main-sequence, subgiant, and giant colour-coded according to the scale on the right-hand side. We also indicate other members without phase estimates in grey.