Finding New Hot Subdwarf Stars in SDSS Images

Hot subdwarf stars, located at the end of the blue horizontal branch, have a burning helium core, and are crucial for studying stellar structure. Currently, the number of known hot subdwarf star is relatively small. Many studies apply machine learning classification to search for hot subdwarf stars...

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Detalhes bibliográficos
Main Authors: Jiangchuan Zhang, Yude Bu, Huili Wu, Yuhang Zhang, Shanshan Li, Zhenxin Lei, Zhenping Yi, Xiaoming Kong, Meng Liu
Formato: Artigo
Idioma:Inglês
Publicado em: IOP Publishing 2025-01-01
Colecção:The Astronomical Journal
Assuntos:
Astronomical object identification
Astrostatistics
Subdwarf stars
Astronomy data analysis
Acesso em linha:https://doi.org/10.3847/1538-3881/adccb5
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