New Teff and [Fe/H] spectroscopic calibration for FGK dwarfs and GK giants
Context. The ever-growing number of large spectroscopic survey programs has increased the importance of fast and reliable methods with which to determine precise stellar parameters. Some of these methods are highly dependent on correct spectroscopic calibrations. Aims: The goal of this work is to obtain a new spectroscopic calibration for a fast
Teixeira, G. D. C. et al.
Advertised on:
10
2016