教育经历
  • 1998-9 — 2002-7
    山东理工大学
    信息与计算科学
    理学学士学位
  • 2002-9 — 2005-3
    上海大学
    计算机及应用
    工学硕士学位
  • 2014-9 — 2018-6
    中国科学院大学
    天文技术与方法
    理学博士学位
工作经历
  • 2022-12 — 2023-12
     天体物理与超级计算中心  斯威本科技大学 
    国家公派访问学者
  • 2019-09 — 2019-11
     英属哥伦比亚大学 
  • 2005-05 — 至今
     山东大学(威海) 
研究概况

机器学习、数据挖掘、光谱分析

论文成果

(1) Zhongding Cheng.Se-ResNet+SVM Model: An Effective Method of Searching for Hot Subdwarfs from LAMOST.The Astrophysical Journal Supplement Series.2024,274 (2):11pp

(2) Fan Wu.Directly Deriving Parameters from SDSS Photometric Images.The Astronomical Journal.2023,166 (88):15pp

(3) Guo, Fengyue.Searching for Barium Stars from the LAMOST Spectra Using the Machine-learning Method:I.The Astronomical Journal.2023,165 (2):40-50

(4) Cai, Beichen.Li-rich Giants Identified from LAMOST DR8 Low-resolution Survey.The Astronomical Journal.2023,165 (2):52-62

(5) Junchao Liang.Estimation of Stellar Atmospheric Parameters with Light Gradient Boosting Machine Algorithm and Principal Component Analysis.The Astronomical Journal.2022,163 (4):153 ~

(6) Minglei Wua.Atmospheric parameter measurement of Low-S/N stellar spectra based on deep learning.Optik.2020,218

(7) MINGLEI WU.Spectra-GANs: A New Automated Denoising Method for Low-S/N Stellar Spectra.IEEE Access.2020,8

(8) Liang, Xilong.A New Moving Group in the Local Arm.Astronomical Journal.2020,159 (5):196-204

(9) Bharat Kumar, Y..s-process abundances of Primary stars in the Sirius-like Systems: Constraints on pollution from AGB stars.IAUS.2019,343 :351-352

(10) Tracing the Origin of Moving Groups. II. Chemical Abundance of Six Stars in the Halo Stream LAMOST-N1.The Astrophysical Journal.2018,868 (2):105-123

(11) Tracing the Origin of Moving Groups. I. The γ Leo Moving Group with High-resolution Spectra from the Subaru Telescope.The Astrophysical Journal.2018,863 (1):4-12

(12) Kong, X. M..Chemical abundances of primary stars in the Sirius-like binary systems.Monthly Notices of the Royal Astronomical Society.2018,476 (1):724-740

(13) Kong, X. M.Three new barium dwarfs with white dwarf companions: BD+68°1027, RE J0702+129 and BD+80°670.Monthly Notices of the Royal Astronomical Society.2018,474 (2):2129-2141

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