VizieR Online Data Catalog: Absolute radial velocities of CARMENES M dwarfs (Lafarga+, 2020)

Absolute radial velocities (RVs) of 323 M dwarf stars observed with CARMENES. The RVs were computed using the cross-correlation function (CCF) method with binary masks on CARMENES visual observations. The RV values and uncertainties also take into account the gravitational redshift and the convective blueshift of the stars. The gravitational redshift is computed using mass and radius values from Schweitzer et al., 2019A&A...625A..68S, Cat. J/A+A/625/A68. We consider the convective blueshift to be 0+/-100m/s for all stars.

(1 data file).