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Fig. 6.

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Similar to Fig. 5 but only using clusters with at least 6 members in the high precision sample. UMAP projections of the stars colouring the real clusters (right), and the groups found by HDBSCAN (left). The stars highlighted in black circles are those recovered in a group with at least 40% homogeneity and completeness (those in boldface in Table 3).

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