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Stellar parameters with FASMA: a new spectral synthesis package

Published online by Cambridge University Press:  07 March 2018

M. Tsantaki ,
D. T. Andreasen ,
G. D. C. Teixeira ,
S. G. Sousa ,
N. C. Santos ,
E. Delgado-Mena  and
G. Bruzual
M. Tsantaki
Affiliation:
Instituto de Radioastronomía y Astrofísica, UNAM, Campus Morelia, A.P. 3-72, C.P. 58089, Michoacán, Mexico email: mtsantaki@crya.unam.mx
D. T. Andreasen
Affiliation:
Instituto de Astrofísica e Ciências do Espaço, Universidade do Porto, CAUP, Rua das Estrelas, Porto, 4150-762, Portugal
G. D. C. Teixeira
Affiliation:
Instituto de Astrofísica e Ciências do Espaço, Universidade do Porto, CAUP, Rua das Estrelas, Porto, 4150-762, Portugal
S. G. Sousa
Affiliation:
Instituto de Astrofísica e Ciências do Espaço, Universidade do Porto, CAUP, Rua das Estrelas, Porto, 4150-762, Portugal
N. C. Santos
Affiliation:
Instituto de Astrofísica e Ciências do Espaço, Universidade do Porto, CAUP, Rua das Estrelas, Porto, 4150-762, Portugal
E. Delgado-Mena
Affiliation:
Instituto de Astrofísica e Ciências do Espaço, Universidade do Porto, CAUP, Rua das Estrelas, Porto, 4150-762, Portugal
G. Bruzual
Affiliation:
Instituto de Radioastronomía y Astrofísica, UNAM, Campus Morelia, A.P. 3-72, C.P. 58089, Michoacán, Mexico email: mtsantaki@crya.unam.mx
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Abstract

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Current Galactic surveys, including the Gaia mission, rely on the efficiency of the spectral analysis techniques to provide precise and accurate spectral information (i.e. effective temperature, surface gravity, metallicity, and chemical abundances) in the shortest computational time. In this work, we present a new package to preform complete spectral analyses based on the spectral synthesis technique (Tsantaki et al. 2017, submitted). We focus on deriving atmospheric parameters for FGK-type stars using both high and medium resolution (GIRAFFE) spectra. This method is implemented on the Gaia-ESO benchmark stars to confirm its validity, achieving similar accuracy for the two resolution setups.

Keywords

techniques: spectroscopicstars: atmospheresfundamental parameters
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 12 , Symposium S330: Astrometry and Astrophysics in the Gaia sky , April 2017 , pp. 271 - 272
Copyright
Copyright © International Astronomical Union 2018 

References

Andreasen, D. T., Sousa, S. G., Tsantaki, M., et al., 2017, A&A, 600, A69 Google Scholar
Blanco-Cuaresma, S., Soubiran, C., Jofré, P., & Heiter, U., 2014, A&A, 566, A98 Google Scholar
Gustafsson, B., Edvardsson, B., Eriksson, K., et al., 2008, A&A, 486, 951 Google Scholar
Hawkins, K., Jofré, P., Heiter, U., et al., 2016, A&A, 592, A70 Google Scholar
Heiter, U., Jofré, P., Gustafsson, B., et al., 2015, A&A, 582, A49 Google Scholar
Jofré, P., Heiter, U., Soubiran, C., et al., 2014, A&A, 564, A133 Google Scholar
Kurucz, R. L. 1993, Kurucz CD-ROM, Cambridge, Smithsonian Astrophysical ObservatoryGoogle Scholar
Mészáros, S., Allende Prieto, C., Edvardsson, B., et al., 2012, ApJ, 144, 120 CrossRefGoogle Scholar
Sneden, C., 1973, ApJ, 184, 839 CrossRefGoogle Scholar
Tsantaki, M., Andreasen, D. T., Teixeira, G. D., Sousa, S. G., et al. 2017 (submitted), MNRAS Google Scholar