Fig. 3
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Modelled properties of stars within the sample (left for NGC 1261 and right for NGC 1904) as a function of ϕ1. As in Fig. 2, each point is colour-coded according to its membership probability of belonging to the respective cluster. The bottom two panels show the histograms of all probabilities in the sample. The vertical lines at 0.6 (60%) represent the threshold on the probability.
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