Fig. B.1
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Zoom into the CMD region with an overlap of the KMOS follow-up with Gaia data. The sources in our catalog are shown as grey dots, previously confirmed members from astrometry, spectroscopy, mid-infrared excess, or X-ray emission as blue stars (Peterson et al. 2011; Galli et al. 2020a; Esplin & Luhman 2022), and objects rejected in (Galli et al. 2020a) as orange crosses. The sources with spectroscopy with KMOS are marked with black circles.
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