ODUSSEAS: Observing Dwarfs Using Stellar Spectroscopic Energy-Absorption Shapes

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Ada Coda
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ODUSSEAS: Observing Dwarfs Using Stellar Spectroscopic Energy-Absorption Shapes

Post by Ada Coda » Thu Feb 27, 2020 3:41 am

ODUSSEAS: Observing Dwarfs Using Stellar Spectroscopic Energy-Absorption Shapes

Abstract: ODUSSEAS (Observing Dwarfs Using Stellar Spectroscopic Energy-Absorption Shapes) uses machine learning to derive the Teff and [Fe/H] of M dwarf stars by using their optical spectra obtained by different spectrographs with different resolutions. The software uses the measurement of the pseudo equivalent widths for more than 4000 stellar absorption lines and the machine learning Python package scikit-learn (https://scikit-learn.org/stable/) to predict the stellar parameters.

Credit: Antoniadis-Karnavas, A.; Sousa, S. G.; Delgado-Mena, E.; Santos, N. C.; Teixeira, G. D. C.; Neves, V.

Site: https://github.com/AlexandrosAntoniadis/ODUSSEAS
https://ui.adsabs.harvard.edu/abs/2020arXiv200209367A

Bibcode: 2020ascl.soft02005A

Preferred citation method: https://ui.adsabs.harvard.edu/abs/2020arXiv200209367A

ID: ascl:2002.005

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