[1]Bu Yude, Du J. The RH boundary value problem of the k-monogenic functions[J]. Journal of mathematical analysis and applications, 2008, 347(2): 633-644.
[2]Bu Yude, Jingchang Pan, Bin Jiang, et al. Spectral feature extraction based on the DCPCA method[J]. Publications of the Astronomical Society of Australia, 2013, 30: e24.
[3]Bu Yude, Jingchang P, Bin J, et al. Stellar Spectral Subclass Classification Based on Locally Linear Embedding[J]. Publications of the Astronomical Society of Japan, 2013, 65(4): 81.
[4]Fuqiang Chen, Yan Wu, Bu Yude, et al. Spectral classification using restricted Boltzmann machine[J]. Publications of the Astronomical Society of Australia, 2014, 31: e001.
[5]卜育德, 潘景昌, 陈福强. 基于 lsomap 算法的恒星光谱离群点挖掘[J]. 光谱学与光谱分析, 2014, 34(1): 267-273.
[6]Bu Yude, Pan J C, Wang J. Estimation of Alpha-Element Abundance Ratios Based on Gaussian Process Regression[J]. Applied Mechanics and Materials, 2014, 543: 1685-1688.
[7]Bu Yude, Chen F, Pan J. Stellar spectral subclasses classification based on Isomap and SVM[J]. New Astronomy, 2014, 28: 35-43.
[8]Bu Yude, Pan J. Stellar atmospheric parameter estimation using Gaussian process regression[J]. Monthly Notices of the Royal Astronomical Society, 2015, 447(1): 256-265.
[9]Bu Yude, Zhao G, Luo A, et al. Restricted Boltzmann machine: a non-linear substitute for PCA in spectral processing[J]. Astronomy & Astrophysics, 2015, 576: A96.
[10]Bu Yude, Zhao G, Pan J, et al. ELM: An Algorithm to estimate the alpha abundance from low-resolution spectra[J]. The Astrophysical Journal, 2016, 817(1): 78.
[11]卜育德, 潘景昌, 王春雨, 等. 基于 LASSO 算法的恒星 α 元素丰度估计方法研究[J]. 光谱学与光谱分析, 2017, 37(1): 278-282.
[12]Bu Yude, Lei Z, Zhao G, et al. Searching for hot subdwarf stars from the LAMOST spectra. I. Method[J]. The Astrophysical Journal Supplement Series, 2017, 233(1): 2.
[13]Lei Zhenxin, Bu Yude, Zhao Jingkun, et al. Searching for hot subdwarf stars from the LAMOST Spectra. II. Pure spectroscopic identification method for hot subdwarfs[J]. Publications of the Astronomical Society of Japan, 2019, 71(2): 41.
[14]王晶, 衣振萍, 岳丽丽, 董慧芬, 潘景昌, 卜育德. 基于集成树的 M 型星光谱分类[J]. 光谱学与光谱分析, 2019, 39(7): 2288-2292.
[15]卜育德, 潘景昌, 衣振萍. 中低分辨率光谱的恒星 I0 元素丰度估计方法研究[J]. 2019.
[16]Bu Yude, Zeng J, Lei Z, et al. Searching for Hot Subdwarf Stars from the LAMOST Spectra. III. Classification of Hot Subdwarf Stars in the Fourth Data Release of LAMOST Using a Deep Learning Method[J]. The Astrophysical Journal, 2019, 886(2): 128.
[17]Wu M, Bu Yude, Pan J, et al. Spectra-gans: A new automated denoising method for low-s/n stellar spectra[J]. IEEE Access, 2020, 8: 107912-107926.
[18]Bu Yude, Kumar Y B, Xie J, et al. Estimation of stellar ages and masses using gaussian process regression[J]. The Astrophysical Journal Supplement Series, 2020, 249(1): 7.
[19]Xie J, Bu Yude, Liang J, et al. Improve the Search of Very Metal-poor Stars Using the Deep Learning Method[J]. The Astronomical Journal, 2021, 162(4): 155.
[20]Cai B, Kong X, Shi J, Gao Q, Bu Yude, Yi Z. Li-rich Giants Identified from LAMOST DR8 Low-resolution Survey[J]. The Astronomical Journal, 2023, 165(2): 52.
[21]Guo F, Cheng Z, Kong X, Zhang Y, Bu Yude, Yi Z, et al. Searching for Barium Stars from the LAMOST Spectra Using the Machine-learning Method: I[J]. The Astronomical Journal, 2023, 165(2): 40.
[22]Minglei W, Jingchang P, Zhenping Y, Xiaoming K, Bu Yude. Atmospheric parameter measurement of Low-S/N stellar spectra based on deep learning[J]. Optik, 2020, 218: 165004.
[23]Zhongding C, Tianmin W, Bu Yude, et al. Se-ResNet+ SVM model: an effective method of searching for hot subdwarfs from LAMOST[J]. arXiv preprint arXiv:2212.10372, 2022.
[24]Liu W, Bu Yude, Kong X, et al. Identifying hot subdwarf stars from photometric data using Gaussian mixture model and graph neural network[J]. arXiv preprint arXiv:2212.10072, 2022.
[25]Liang J, Bu Yude, Tan K, et al. Estimation of stellar atmospheric parameters with light gradient boosting machine algorithm and principal component analysis[J]. The Astronomical Journal, 2022, 163(4): 153.
[26]Yi Z, Li J, Du W, Liu M, Liang Z, Xing Y, Pan J, Bu Yude, et al. Automatic detection of low surface brightness galaxies from Sloan Digital Sky Survey images[J]. Monthly Notices of the Royal Astronomical Society, 2022, 513(3): 3972-3981.
[27]Wu F, Bu Yude, Zhang M, et al. Directly Deriving Parameters from SDSS Photometric Images[J]. The Astronomical Journal, 2023, 166(3): 88.
[28]Bai S. C, Shi Q, Zhang H, Guo R, Shen X. C, Liu T. Z, Degeling A. W, Tian A, Bu Yude, et al. Electron Dynamics and Whistler‐Mode Waves Inside the Short Large‐Amplitude Magnetic Field Structures[J]. Journal of Geophysical Research: Space Physics, 2023, 128(11): e2023JA031816.
[29]Wu T, Bu Yude, Xie J, et al. Estimating stellar parameters and identifying very metal-poor stars for low-resolution spectra (R∼ 200)[J]. Publications of the Astronomical Society of Australia, 2024, 41: e002.
[30]Wu M, Bu Yude. Defective flux and splicing abnormality restoration of stellar spectra in LAMOST based on deep learning[J]. Publications of the Astronomical Society of Japan, 2025, 77(1): 46-60.
[31]Zhang J, Bu Yude, Zhang M, et al. A Multiple-detection-heads Machine Learning Algorithm for Detecting White Dwarfs[J]. The Astrophysical Journal Supplement Series, 2025, 276(2): 53.
[32]Bai S, Guo R, Xiao Y, Shi Q, Yao Z, Pu Z, Sun W, Degeling A. Tian A, Rae I, Yao S, Zong Q, Fu S, Bu Yude et al. Spontaneously generated flux ropes in 3‐D magnetic reconnection[J]. Journal of Geophysical Research: Space Physics, 2025, 130(1): e2024JA033461.
[33]Wu H, Bu Yude, Zhang J C, et al. Search for hot subdwarf stars from SDSS images using a deep learning method: SwinBayesNet[J]. Astronomy & Astrophysics, 2025, 693: A245.
[34]Wu H, Bu Yude, Zhang J, et al. VizieR Online Data Catalog: Catalog of hot subdwarf candidates (Wu+, 2025)[J]. VizieR Online Data Catalog, 2024, 369: J/A+ A/693/A245.
[35]Zhang M, Bu Yude, Wu F, et al. The impact of UV spectra on searches for extremely metal-poor stars: A study for future CSST observations[J]. Astronomy & Astrophysics, 2024, 691: A21.
[36]Song S, Kong X, Bu Yude, et al. MEASNet. I. A Model for Barium Star Identification and s-process Abundance Estimation from LAMOST DR10 Low-resolution Survey[J]. The Astrophysical Journal, 2024, 974(1): 78.
[37]Cheng Z, Kong X, Wu T, Zhang A, Liu B, Bu Yude et al. Se-ResNet+ SVM Model: An Effective Method of Searching for Hot Subdwarfs from LAMOST[J]. The Astrophysical Journal Supplement Series, 2024, 274(1): 2.
[38]Liang Z, Yi Z, Du W, Liu M, Liu Y, Wang J, Kong X, Bu Yude, et al. Automatic Search for Low-surface-brightness Galaxies from Sloan Digital Sky Survey Images Using Deep Learning[J]. The Astronomical Journal, 2024, 168(2): 74.
[39]Xie D, Zhang J, Bu Yude, et al. An adaptive parameter estimator for poor-quality spectral data of white dwarfs[J]. arxiv preprint arxiv:2406.04248, 2024.
[40]Liu W, Bu Yude, Kong X, et al. Identifying hot subdwarf stars from photometric data using a Gaussian mixture model and graph neural network[J]. Publications of the Astronomical Society of Japan, 2024, 76(3): 329-339.
[41]Zhang R, Liu M, Yi Z, Yuan H, Yang Z, Bu Yude, et al. Deblending overlapping galaxies in DECaLS using transformer-based algorithm: A method combining multiple bands and data types[J]. Publications of the Astronomical Society of Australia, 2024, 41: e035.
[42]Bai S C, Shi Q, Shen X C, Tian A, Zhang H, Guo R, Wang M, Degeling A, Bu Yude, et al. Whistler‐mode waves inside short large‐amplitude magnetic field structures: Characteristics and generation mechanisms[J]. Journal of Geophysical Research: Space Physics, 2024, 129(3): e2023JA032392.
[43]Zhang M, Wu F, Bu Yude, et al. SPT: Spectral transformer for age and mass estimations of red giant stars[J]. Astronomy & Astrophysics, 2024, 683: A163.
[44]Xing Y, Yi Z, Liang Z, Su H, Du W He M, Liu M, Kong X, Bu Yude, et al. VizieR Online Data Catalog: Low-surface-brightness galaxy cand. from SDSS DR16 (Xing+, 2023)[J]. VizieR Online Data Catalog, 2024, 226: J/ApJS/269/59.
[45]Su H, Yi Z, Liang Z, Du W, Liu M, Kong X, Bu Yude, et al. LSBGnet: an improved detection model for low-surface brightness galaxies[J]. Monthly Notices of the Royal Astronomical Society, 2024, 528(1): 873-882.
[46]Zhang M, Wu F, Bu Yude, et al. Spt: Spectral transformer for red giant stars age and mass estimation[J]. arxiv preprint arxiv:2401.04900, 2024.
[47]Xing Y, Yi Z, Liang Z, Su H, Du W, He M, Liu M, Kong X, Bu Yude, Wu H. Edge-on Low-surface-brightness Galaxy Candidates Detected from SDSS Images Using YOLO[J]. The Astrophysical Journal Supplement Series, 2023, 269(2): 59.
[48]Yuan H, Liu M, Yang Z, Bu Yude, et al. Red Giants Search Method Based on Convolutional Neural Networks[J]. The Astronomical Journal, 2023, 166(6): 244.
[49]Yang Z, Liu M, Yuan H, Bu Yude, et al. Star Photometry for DECam Legacy Survey and Sloan Digital Sky Survey Images Based on Convolutional Neural Networks[J]. The Astronomical Journal, 2023, 166(5): 210.
[50]Bai S C, Shi Q, Zhang H, Guo R, Shen X, Liu T Z, Degeling A Tian M, Bu Yude, et al. Electron dynamics and whistler‐mode waves inside the short large‐amplitude magnetic field structures[J]. Journal of Geophysical Research: Space Physics, 2023, 128(11): e2023JA031816.
[51]Cao Z, Yi Z, Pan J, Su H, Bu Yude, et al. L-Dwarf Detection from SDSS Images Using Improved Faster R-CNN[J]. The Astronomical Journal, 2023, 165(4): 184.
[52]Li X, Bu Yude, Xie J, et al. Determine the Masses and Ages of Red Giant Branch Stars from Low-resolution LAMOST Spectra Using DenseNet[J]. arxiv preprint arxiv:2106.04945, 2021.
