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Detection of hot subdwarf binaries and He-poor hot subdwarf stars using machine learning methods and a large sample of Gaia XP spectra | Astronomy & Astrophysics (A&A)
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Home All issues Volume 708 (April 2026) A&A, 708 (2026) A23 Full HTML
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Fig. A.7

Fig. A.7 Refer to the following caption and surrounding text.

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PR curves for different models and classification tasks.

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