VizieR Online Data Catalog: Radii and masses of the CARMENES targets (Schweitzer+, 2019)

Table B1 contains the stellar parameters of our sample. The sample consists of 293 nearby, bright M dwarfs with no known close companions. Their metallicities spread around solar metallicity. Most stars are inactive or mildly active and older than a few hundred million years. However, known active or young stars are also included although most of the analyses assume inactive main sequence stars. All parameters are determined by us except where noted otherwise.

(1 data file).