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Tutorial: Measuring Stellar Atmospheric Parameters with ARES+MOOG

  • Sérgio G. SousaEmail author
  • Daniel T. Andreasen
Conference paper
Part of the Astrophysics and Space Science Proceedings book series (ASSSP, volume 49)

Abstract

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.

Notes

Acknowledgements

SGS and DTA acknowledge the support from Fundação para a Ciência e a Tecnologia (FCT) through national funds and a research grant (project ref. UID/FIS/04434/2013, PTDC/FIS-AST/7073/2014, and grant ref. CAUP-09/2014-BD). SGS also acknowledges the support from FCT through Investigador FCT contract with reference IF/00028/2014 and POPH/FSE (EC) by FEDER funding through Programa Operacional de Factores de Competitividade COMPETE.

References

  1. Gray, D.F.: The Observation and Analysis of Stellar Photospheres. Cambridge University Press, Cambridge (2008)Google Scholar
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  5. Sousa, S.G., Santos, N.C., Adibekyan, V., Delgado-Mena, E., Israelian, G.: Astron. Astrophys. 577, A67 (2015)ADSCrossRefGoogle Scholar

Copyright information

© Springer International Publishing AG 2018

Authors and Affiliations

  1. 1.Instituto de Astrofísica e Ciências do EspaçoUniversidade do Porto, CAUPPortoPortugal

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