基于解耦训练的脉冲星识别算法
[1] Hewish A, Bell S J, Pilkington J D H, et al. Observation of a rapidly pulsating radio source[M]∥A Source Book in Astronomy and Astrophysics, 1900-1975. Cambridge: Harvard University Press,2013:498-504.
[2] 张承民. 中国天眼科普:神秘的脉冲星[M]. 北京:清华大学出版社,2019.
[3] 帅平, 陈绍龙, 吴一帆, 等. X 射线脉冲星导航原理[J]. 宇航学报,2007(6):1538-1543.
[4] Hobbs G, Miller D, Manchester R N, et al. The parkes observatory pulsar data archive[J]. Publications of the Astronomical Society of Australia,2011,28(3):202-214.
[5] Radford A, Metz L, Chintala S. Unsupervised representation learning with deep convolutional generative adversarial networks[EB/OL].(2016-01-07)[2022-05-31].https:∥airxiv.org/abs/1511.06434.
[6] 刘晓飞, 劳保强, 安涛, 等. 基于深层残差网络的脉冲星候选体分类方法研究[J].天文学报,2021,62(2):98-111.
[7] 王元超, 郑建华, 潘之辰, 等. 脉冲星候选样本分类方法综述[J].深空探测学报,2018,5(3):203-211.
[8] 王洪丰. 基于机器学习的脉冲星搜寻方法研究[D].北京:北京师范大学,2020.
[9] Morello V, Barr E D, Bailes M, et al. SPINN: a straightforward machine learning solution to the pulsar candidate selection problem[J]. Monthly Notices of the Royal Astronomical Society,2014,443(2):1651-1662.
[10] Guo P, Duan F, Wang P, et al. Pulsar candidate classification using generative adversary networks[J]. Monthly Notices of the Royal Astronomical Society,2019,490(4):5424-5439.
[11] Boyan Zhou, Quan Cui, Xinshen Wei, et al. BBN: Bilateral-branch network with cumulative learning for long-tailed visual recognition[C]∥IEEE Conference on Computer Vision and Pattem Recogition,2020.
[12] Chang C C, Lin C J. LIBSVM: a library for support vector machines[J]. ACM transactions on intelligent systems and technology (TIST),2011,2(3):1-27.
[13] Shlens J. A tutorial on principal component analysis[EB/OL].(2014-03-03)[2022-05-31].https:∥arxiv.org/abs/1404.1100.
[14] Chang C C, Lin C J. LIBSVM: a library for support vector machines[J]. ACM transactions on intelligent systems and technology (TIST),2011,2(3):1-27.
尹乾, 车润琪, 杨如意, 郑新. 基于解耦训练的脉冲星识别算法[J]. 光学技术, 2023, 49(6): 680. YIN Qian, CHE Runqi, YANG Ruyi, ZHENG Xin. Pulsar recognition algorithm based on decoupling training[J]. Optical Technique, 2023, 49(6): 680.