Predicting Stellar Parameters of Massive Stars from Light Curves with Machine Learning

High-resolution spectroscopic measurements of OB stars are important for understanding processes like stellar evolution but require labor-intensive observations. In contrast, photometric missions like the Transiting Exoplanet Survey Satellite (TESS) can monitor hundreds of thousands of stars with a...

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Hlavní autoři:	Rachel C. Zhang, Kaze W. K. Wong, Gonzalo Holgado, Matteo Cantiello
Médium:	Artigo
Jazyk:	Inglês
Vydáno:	IOP Publishing 2025-01-01
Edice:	The Astrophysical Journal
Témata:	Stellar astronomy Astronomy data analysis Massive stars
On-line přístup:	https://doi.org/10.3847/1538-4357/ae1d70
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