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astro-ph.SR2025
A robust method for identifying Be stars in the LAMOST Data Release 11 based on Deep-learning approach
Lei Tan, Hui Deng, Ying Mei +4
Be stars are rapidly rotating B-type stars that exhibit Balmer emission lines in their optical spectra. These stars play an important role in studies of stellar evolution and disk…
astro-ph.SR2022★ 17 cited
Identify 46 New Open Clusters Candidates In Gaia EDR3 Using pyUPMASK and Random Forest Hybrid Method
Huanbin Chi, Shoulin Wei, Feng Wang +1
Open clusters (OCs) are regarded as tracers to understand stellar evolution theory and validate stellar models. In this study, we presented a robust approach to identifying OCs. A…