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Paper: Fundamental Physical Parameters Estimation of O-type Stars Using Artificial Neural Networks
Volume: 538, ADASS XXXII
Page: 269
Authors: Miguel Flores R.; Luis J. Corral; Celia R. Fierro-Santillán; Silvana G. Navarro
DOI: 10.26624/NGZN1317
Abstract: We present an artificial neural network approach to estimating stellar luminosity, effective temperature, and surface gravity. The project’s final objective is to develop a system capable of automatically fitting stellar spectra models and determining the physical parameters of the stars. In previous work, we tried to establish the best way to fit a stellar model using different machine-learning models and two primary methods: the classification of the stellar spectra models and estimates of physical parameters in a regression-type task. Here, we present the results of implementing a set of recurrent neural networks trained with a database of synthetic model spectra and the predictions of O-type stars’ observed spectra.
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