Stellar atmospheric parameters of CARMENES GTO M-dwarfs with spectral synthesis and SteParSyn
We aim to review the spectral synthesis technique to derive the stellar atmospheric parameters (T eff, log g, and [Fe/H]) of 348 M dwarfs in light of the optical and near-infrared spectra obtained with CARMENES, the high-resolution, double-channel spectrograph installed at the 3.5 m telescope at the Calar Alto observatory (Spain). The analysis
Marfil, Emilio et al.
Fecha de publicación:
3
2021