Best isochrone fittings for all clusters. Left panels: cluster stars according to the membership probabilities (p_member). Right panels: synthetic CMD-generated parameters found for the best solution. The number of points is equal to the observed CMDs within the same magnitude limits. The horizontal dashed lines correspond to the magnitude limits used to compute the likelihood (brighter mag) and p_member (fainter mag). The solid blue line correspond to the PARSEC isochrones with the parameters found in Table 5.