Fig. 2.
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CMD for all the measured stars in the field of NGC 6362, with their respective photometric errors. Black and gray dots represent stars located inside and outside a circle of radius equals to two times the cluster’s half-mass radius (0.11 deg), respectively. The red line is an isochrone for the cluster’s age (12 Gyr) and metallicity ([Fe/H] = −1.07 dex) (Gontcharov et al. 2023).
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