Fig. 7
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Color-magnitude diagrams of our sample of nearby red-dwarf candidates (in red) compared with the entire Gaia Catalog of Nearby Stars shown in blue. From left to right, G vs (BP – RP), Ks vs (J – Ks) and Ks vs (G – Ks) diagrams are shown. In the three plots, our objects are located at the faintest magnitudes, and are mainly clustered in the main sequence.
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