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Fig. 5.

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UMAP projections of the stars in the high-precision sample. The groups are coloured according to whether they were found by HDBSCAN (left) or are real clusters (right). The grey points correspond to stars that were found as noise. The stars highlighted with black circles were recovered in a group with at least 40% homogeneity and completeness (those in boldface in Table 2), and the corresponding cluster is labelled.

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