Left: color-magnitude diagram of all low-mass (0.7 − 2.3 M_⊙) RG candidates within 200 pc (blue dots) from Gaia DR2 for the southern hemisphere stars. As a comparison, the Gaia DR2 color-magnitude diagram of the 100 pc clean sample (sample C in Lindegren et al. 2018) is shown in gray. The slightly larger gray dots within the selected sample represent the low-mass RG candidates within 500 pc. The red circles show the low-mass RG candidates that were observed with EULER/CORALIE. Right: sky locations (Galactic coordinates, Aitoff projection) of the volume-limited low-mass RG sample within 200 pc with respect to the galactic coordinate system use the same color-coding.