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On the Use of Logistic Regression for stellar classification. An application to colour-colour diagrams

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arxiv 1805.09551 v1 pith:ZOTOUNRX submitted 2018-05-24 astro-ph.SR

On the Use of Logistic Regression for stellar classification. An application to colour-colour diagrams

classification astro-ph.SR
keywords classificationalgorithmsappliedcolour-colourdatadiagramslogisticmethod
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We are totally immersed in the Big Data era and reliable algorithms and methods for data classification are instrumental for astronomical research. Random Forest and Support Vector Machines algorithms have become popular over the last few years and they are widely used for different stellar classification problems. In this article, we explore an alternative supervised classification method scarcely exploited in astronomy, Logistic Regression, that has been applied successfully in other scientific areas, particularly biostatistics. We have applied this method in order to derive membership probabilities for potential T Tauri star candidates from ultraviolet-infrared colour-colour diagrams.

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  1. Effective temperatures estimation of low-mass stars and identification of T Tauri stars in LAMOST DR10 using machine learning

    astro-ph.SR 2026-07 conditional novelty 5.0

    A GBM regressor trained on PHOENIX synthetic spectra estimates Teff for 1,733,852 LAMOST DR10 low-mass spectra, and a robust logistic classifier identifies 2,534 T Tauri star candidates.