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Fig. 17

image

Left column: top, MPs distribution for an old SOC where the cut is done for a value of probmin = 0.75; center, CMD of cluster region with MPs for each star shown according to the color bar at the top and the best-fit isochrone found shown in green; bottom, best-fit synthetic cluster found along with the theoretical isochrone used to generate it in red, cluster parameters and uncertainties shown in the top right box. Right column: top, idem above with probability cut now done at probmin = 0.85; center, idem above with new best-fit isochrone; bottom, idem above showing new synthetic cluster and improved cluster parameters.

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