S. G. Sousa, D. T. Andreasen
The technical aspects of using an Equivalent Width (EW) method for the derivation of spectroscopic stellar parameters with ares+moog are described herein. While the science background to this method can be found in numerous references, the goal here is to provide a user-friendly guide to the several codes and scripts used in the tutorial presented at the School. All the required data have been made available online at the following repository: https://github.com/sousasag/school_codes.
Asteroseismology and Exoplanets: Listening to the Stars and Searching for New Worlds
Tiago L. Campante, Nuno C. Santos, Mário J. P. F. G. Monteiro
Series Astrophysics and Space Science Proceedings
Volume 49, Page 275