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Fig. C.1.

image

Left panel: proper motion diagram of the sources selected in the region defined in the text. Proper motions cluster at μα*, μδ ∼ ( − 7., − 2.5) mas yr−1, with a few scattered outliers. Centre panel: parallax histogram of the candidate cluster members. The histogram peaks at ϖ ∼ 3.4 mas, indicating a distance to the cluster of ∼295 pc. Right panel: corrected colour-magnitude diagram of the candidate cluster members. The 10, 15, and 20 Myr PARSEC isochrones with solar metallicity and AV = 0 mag are also plotted as grey solid lines.

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