Context. Being the most numerous and oldest stars in the galaxy, M dwarfs are objects of
great interest for exoplanet searches. The presence of molecules in their atmosphere
complicates our understanding of their atmospheric properties. But great advances have
recently been made in the modeling of M dwarfs due to the revision of solar abundances.
Aims. We aim to determine stellar parameters of M dwarfs using high resolution spectra (R∼
90 000) simultaneously in the visible and the near-infrared. The high resolution spectra and …

–Caption of Fig. 5: References to right and left panels are inverted. The corrected figure
caption is: Left panel: comparison of Teff versus spectral type relation as a function of
metallicity from this study with Passegger et al.(2018; open triangle) and with Rajpurohit et
al.(2013; open circle). Right panel: comparison of Teff determined from this study with
Passeggeretal.(2018; open triangle) and with Gaidos & Mann (2014; filled square) as
function of metallicity.–Corrected text (page 5, right column): In order to explore the effect of …