Stellar atmospheric parameters of FGK-type stars from high-resolution optical 
and near-infrared CARMENES spectra

Marfil, E.; Montes, D.; Tabernero, H. M.; Caballero, J. A.; González Hernández, J. I.; Kaminski, A.; Simón-Díaz, S.; Jeffers, S. V.; Quirrenbach, A.; Amado, P. J.; Ribas, I.; Reiners, A.; Seifert, W.; Consortium, CARMENES

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Stellar atmospheric parameters of FGK-type stars from high-resolution optical and near-infrared CARMENES spectra

MPS-Authors

Marfil, E.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Montes, D.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Tabernero, H. M.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Caballero, J. A.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

González Hernández, J. I.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Kaminski, A.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Simón-Díaz, S.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Jeffers, S. V.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Quirrenbach, A.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Amado, P. J.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Ribas, I.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Reiners, A.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Seifert, W.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Consortium, CARMENES
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

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https://ui.adsabs.harvard.edu/abs/2019hsax.conf..409M
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Citation

Marfil, E., Montes, D., Tabernero, H. M., Caballero, J. A., González Hernández, J. I., Kaminski, A., et al. (2019). Stellar atmospheric parameters of FGK-type stars from high-resolution optical and near-infrared CARMENES spectra.

Cite as: https://hdl.handle.net/21.11116/0000-0005-D301-B

Abstract

With the aim of using classic spectroscopic methods with high resolution and high signal-to-noise ratio in the NIR spectral window, we made a selection of 66 FGK-type stars observed with CARMENES, the brand-new, ultra-stable, double-channel spectrograph at the Spanish-German 3.5m Calar Alto telescope. These spectra are part of a CARMENES stellar library. We applied the equivalent width method to derive the spectroscopic stellar parameters (T_{eff}, log{g}, {ξ}_{micro}, and [Fe/H]) using the StePar code along with four new iron line lists covering the whole CARMENES spectral range (550 - 1700 nm).