Fig. 4.
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Raw CMD diagrams for the three clusters observed, based on Gaia photometry. From left to right: UBC 103, UBC 114, and UBC 587 (noting the shift in the horizontal axis due to higher extinction). The large striped circles indicate the stars whose spectra were collected. Cluster members are from Cantat-Gaudin et al. (2020). See main text for details.
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