1. Bu Yude, Du Jinyuan. The RH boundary value problem of the k-monogenic functions of the k- monogenic functions. Journal of Mathematical Analysis and Application(347) 2008,633-644.
2. Yude Bu, Gang Zhao, Jingchang Pan, and Yerra Bharat Kumar, ELM: An Algorithm to estimate the alpha abundance from low-resolution spectra, The Astrophysical Journal, 2016, 817, 78:1-10
3. Bu Yude, Pan Jingchang, Stellar atmospheric parameter estimation using Gaussian process regression, Monthly Notices of the Royal Astronomical Society, 2015, 447(1):256-265
4. Bu Yude, Zhao Gang, Luo A-Li, Pan Jingchang, Chen Yuqin, Restricted Boltzmann machine: a non-linear substitute for PCA in spectral processing, Astronomy & Astrophysics, 2015, 576, A96:1-8
5. Bu Yude, Pan Jingchang, Jiang Bin, Chen Fuqiang and Wei Peng, Spectral Feature Extraction Based on the DCPCA Method, Publications of the Astronomical Society of Australia (PASA),2013, 30, e24:1-16
6. Yude Bu, Jingchang Pan, Bin Jiang and Peng Wei, Stellar Spectral Subclass Classification Based on Locally Linear Embedding, Publications of the Astronomical Society of Japan,2013, 65(4):1-16
7. Bu Yude, Fuqiang Chen and Jingchang Pan, Stellar spectral subclasses classification based on Isomap and SVM, New Astronomy, 2014, 28:35-43
8. Bu Y D, Pan J C, Wang J. Estimation of Alpha-Element Abundance Ratios Based on Gaussian Process Regression, Applied Mechanics & Materials, 2014, 543-547:1685-1688
9. Chen Fuqiang, Wu Yan, Bu Yude and Zhao Guodong, Spectral Classification Using Restricted Boltzmann Machine, Publications of the Astronomical Society of Australia (PASA), 2014, 31 , id.e001,
10. Bu Yude, Lei Z, Zhao Gang, Bu Jingde, Pan Jingchang, et al. Searching for Hot Subdwarf Stars from the LAMOST Spectra. I. Method[J]. Astrophysical Journal Supplement, 2017, 233(1):2：1-10
11. Bu Yude, Pan Jingchang, Yi Zhenping, Estimating of Mgabundance from low resolution spectra Using ELM algorithm, Sepctroscopic and Spectral analysis. 2019,39(10)：3288-329
12. Lei Z, Bu Y, Zhao J, NémethP, Zhao G. Searching for hot subdwarf stars from the LAMOST Spectra. II. Purespectroscopic identification method for hot subdwarfs. Publications of theAstronomical Society of Japan. 2019, 11;71(2):41.
13. Wang Jing, Yi zhenping, Yu Lili, Dong Huifen, Pan Jingchang, Bu Yude, Spectral classification of M-type stars based on Ensemble tree models. Sepctroscopic and Spectral analysis. 2019(7)：2288-2292.
14. BuYude, Zeng Jingjing, Lei Zhenxin, Yi Zhenping, Searching for HotSubdwarf Stars from the LAMOST Spectra. III. Classification of Hot SubdwarfStars in the Fourth Data Release of LAMOST Using a Deep Learning Method. The Astrophysical Journal, 2019.11:886(2),128:1-10. 2019,11,28
