Notes. Stellar properties of our sample of 177 stars. V-K are from the CDS when available, or derived from the relation between G-K versus V-K when V is not available (indicated by “d”). Most distances are from Gaia Collaboration (2018). When not available, distances were derived from the following parallaxes: parallaxes of GJ 257, GJ 2033, GJ 4206, GJ 9163, and HD196982 are from van Leeuwen (2007), the parallax of GJ 406 is from Weinberger et al. (2016), the parallaxes of GJ 3813 and GJ 4038 are from Finch et al. (2018), the parallax of L43-72 is from Winters et al. (2017), and the parallax of LP 993-116 is from Riaz et al. (2006); the distance of GJ 3332 is from Riedel et al. (2014). Masses are from the mass-luminosity relation of Delfosse et al. (2000), with a weighted average of the masses derived from H, K, and J from the CDS: these band magnitudes were taken from the 2MASS database (Cutri et al. 2003) with the exception of H and J for GJ 205 from Ducati (2002), and H of GJ 1 and K of GJ 803 from Koen et al. (2010). T_eff is from the CDS. The flag indicates whether the star is in the season sub-sample. Only the beginning of the table is shown for information. The full table is available online at the CDS.