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Paper: O-type Stars’ Stellar Parameter Estimation with ANN
Volume: 541, ADASS XXXIII
Page: 189
Authors: L.J. Corral; M. Flores; C. Fierro-Santillán; S.G. Navarro
DOI: 10.26624/QIBL1369
Abstract: We present the results of the implementation of a deep learning system capable of estimating the effective temperature and surface gravity of O-type stars. The proposed system was trained with a database of CMFGEN stellar atmosphere code that covers stars with Teff from ∼20,000 K to ∼58,000 K, log g from 2.4 to 4.2 dex, and mass from 9 to 120 M⊙. One of the advantages proposed in this paper include using a set of equivalent width measurements over the optical region of the stellar spectra, which avoids processing the full spectra that allows it to apply the same trained system over different spectra resolutions.
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