July 7, 2014Open Access

Determining stellar atmospheric parameters and chemical abundances of FGK stars with iSpec

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Resumen

Context. An increasing number of high-resolution stellar spectra is available today thanks to many past and ongoing extensive spectroscopic surveys. Consequently, the scientific community needs automatic procedures to derive atmospheric parameters and individual element abundances.

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Blanco-Cuaresma et al. (Mon,) studied this question.

synapsesocial.com/papers/6a20bb4fa66ec54673ab3631 https://doi.org/https://doi.org/10.1051/0004-6361/201423945

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