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Fig. A.1

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TCDs for the clusters Berkeley 86 (left) and NGC 2244 (right). The solid line shows a normal extinction law, while the fitting for the cluster members is shown by a dotted line. Two extinction vectors (AV = 2 mag) related to different values of RV are plotted in the bottom panels, for illustration. Open circles indicate the members and crosses show the stars with P% < Pmin.

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