Fig. 7
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Gaia B P minus R P color vs. absolute magnitude for the model input stars (green region). The FGKM golden sample is shown in yellow. Absolute magnitude is computed as: mG = phot_g_mean_mag + 5.0 · log(parallax)−10. Close binary systems where the smaller companion is a brown dwarf or a giant planet are displayed as diamonds (blue) and NSS Orbital* solutions are displayed as squares (magenta). CARMENES sources are displayed as circles (orange). Sources in correspond to the Gaia Catalog of Nearby Stars within d<100 pc.
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