• DOI:10.1051/0004-6361/202038295
• Corpus ID: 220871254

CARMENES input catalogue of M dwarfs

@article{Cifuentes2020CARMENESIC,
  title={CARMENES input catalogue of M dwarfs},
  author={Carlos Cifuentes and Jos{\'e} A. Caballero and M. Cort{\'e}s-Contreras and David Montes and F J Abell{\'a}n and Ricardo Dorda and G. Holgado and Mar{\'i}a Rosa Zapatero Osorio and J. C. Morales and Pedro J. Amado and V. M. Passegger and Andreas Quirrenbach and Ansgar Reiners and Ignasi Ribas and Jorge Sanz-Forcada and A. Schweitzer and Walter Seifert and Enrique Solano},
  journal={Astronomy \& Astrophysics},
  year={2020}
}

• C. Cifuentes, J. Caballero, +15 authors E. Solano
• Published 29 July 2020
• Physics, Geology
• Astronomy & Astrophysics

Context. The relevance of M dwarfs in the search for potentially habitable Earth-sized planets has grown significantly in the last years.
Aims. In our on-going effort to comprehensively and accurately characterise confirmed and potential planet-hosting M dwarfs, in particular for the CARMENES survey, we have carried out a comprehensive multi-band photometric analysis involving spectral energy distributions, luminosities, absolute magnitudes, colours, and spectral types, from which we have derived basic astrophysical parameters.
Methods. We have carefully compiled photometry in 20 passbands from the ultraviolet to the mid-infrared, and combined it with the latest parallactic distances and close-multiplicity information, mostly from Gaia DR2, of a sample of 2479 K5 V to L8 stars and ultracool dwarfs, including 2210 nearby, bright M dwarfs. For this, we made extensive use of Virtual Observatory tools.
Results. We have homogeneously computed accurate bolometric luminosities and effective temperatures of 1843 single stars, derived their radii and masses, studied the impact of metallicity, and compared our results with the literature. The over 40 000 individually inspected magnitudes, together with the basic data and derived parameters of the stars, individual and averaged by spectral type, have been made public to the astronomical community. In addition, we have reported 40 new close multiple systems and candidates (ρ <  3.3 arcsec) and 36 overluminous stars that are assigned to young Galactic populations.
Conclusions. In the new era of exoplanet searches around M dwarfs via transit (e.g. TESS, PLATO) and radial velocity (e.g. CARMENES, NIRPS+HARPS), this work is of fundamental importance for stellar and therefore planetary parameter determination.