Finally, the lower right panel is CMD of stars satisfying all conditions. Stellar extinction is calibrated for whole stars with Gaia data. Stars without Gaia extinction data were calibrated with average extinction value of other cluster member stars that have data. Blue line is the best fit isochrone line with PARSEC (
http://stev.oapd.inaf.it/cgi-bin/cmd) set of Z=0.02 isochornes.