Fig. 3.
CMD with the selection using Gaia photometry and parallaxes. Two sets of Parsec isochrones (Bressan et al. 2012) of ages 1−14 Gyr and metallicities −0.5 (red) and −1.5 (blue) are shown. The absolute magnitudes were computed assuming the distances of Bailer-Jones et al. (2018).
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