The CARMENES search for exoplanets around M dwarfs. Different roads to radii and masses of the target stars
Aims: We determine the radii and masses of 293 nearby, bright M dwarfs of the CARMENES survey. This is the first time that such a large and homogeneous high-resolution (R > 80 000) spectroscopic survey has been used to derive these fundamental stellar parameters. Methods: We derived the radii using Stefan-Boltzmann's law. We obtained the required
Schweitzer, A. et al.
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2019