• Acta Physica Sinica
  • Vol. 69, Issue 6, 069701-1 (2020)
Zhi-Wei Kang1、*, Tuo Liu1, Jin Liu2, Xin Ma3, and Xiao Chen4
Author Affiliations
  • 1College of Computer Science and Electronic Engineering, Hunan University, Changsha 410082, China
  • 2College of Information Science and Engineering, Wuhan University of Science and Technology, Wuhan 430081, China
  • 3College of Instrument Science and Opto Electronic Engineering, Beihang University, Beijing 100191, China
  • 4Shanghai Institution of Satellite Engineering, Shanghai 200240, China
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    DOI: 10.7498/aps.69.20191582 Cite this Article
    Zhi-Wei Kang, Tuo Liu, Jin Liu, Xin Ma, Xiao Chen. Pulsar candidate selection based on self-normalizing neural networks[J]. Acta Physica Sinica, 2020, 69(6): 069701-1 Copy Citation Text show less
    SELU activation function.
    Fig. 1. SELU activation function.
    GMO_SNN candidate selection algorithm.
    Fig. 2. GMO_SNN candidate selection algorithm.
    Comparison of the loss function between SNN and ANN.
    Fig. 3. Comparison of the loss function between SNN and ANN.
    数据集非脉冲星数脉冲星数总样本数
    HTRU 189996119691192
    HTRU 216259163917898
    LOTAAS 14987665053
    Table 1.

    Pulsar candidate datasets.

    脉冲星候选体数据集

    编号特征编号特征
    1P12轮廓直方图最大值/高斯拟合的最大值
    2DM13对轮廓求导后的直方图与轮廓直方图的偏移量
    3S/N14$S/N/\sqrt {\left( {P - W} \right)/W} $
    4W15拟合 $S/N/\sqrt {\left( {P - W} \right)/W} $
    5用sin曲线拟合脉冲轮廓的卡方值16DM拟合值与DM最优值取余
    6用sin2曲线拟合脉冲轮廓的卡方值 17DM曲线拟合的卡方值
    7高斯拟合脉冲轮廓的卡方值18峰值处对应的所有频段值的均方根
    8高斯拟合脉冲轮廓的半高宽19任意两个频段线性相关度的均值
    9双高斯拟合脉冲轮廓的卡方值20线性相关度的和
    10双高斯拟合脉冲轮廓的平均半高宽21脉冲轮廓的波峰数
    11脉冲轮廓直方图对0的偏移量22脉冲轮廓减去均值后的面积
    Table 2.

    Feature description.

    特征描述

    隐藏层数F1-score/%
    282.48
    489.58
    894.56
    994.20
    Table 3. [in Chinese]
    批次大小F1-score/%运行时间/s
    1694.8774
    3294.5643
    6493.9023
    12891.0511
    Table 4. [in Chinese]
    隐藏层数F1-score/%
    0.1无法收敛
    0.0194.29
    0.00194.55
    0.000184.10
    Table 5. [in Chinese]
    数据集模型Accuracy/%Recall/%Precison/%F1-score/%FPR/%G-mean/%
    HTRU 1SNN99.8292.4493.4592.940.0896.11
    GA_SNN99.8592.4595.1993.800.0696.12
    MO_SNN99.8194.2397.9496.050.0597.05
    GMO_SNNNNNNNNN99.8595.3298.5196.890.0497.61
    HTRU 2SNN98.3087.7393.9390.730.5993.38
    GA_SNN98.3088.9192.8690.840.7193.96
    MO_SNN97.8992.1795.0893.600.9595.54
    GMO_SNNNNNNNNN98.0392.5395.5894.030.0895.78
    LOTAAS 1SNN99.9293.75100.0096.770.0896.79
    GA_SNN99.92100.0093.3396.550100.00
    MO_SNN99.69100.0087.1093.100.3199.84
    GMO_SNN100.00100.00100.00100.000100.00
    Table 6. [in Chinese]
    Zhi-Wei Kang, Tuo Liu, Jin Liu, Xin Ma, Xiao Chen. Pulsar candidate selection based on self-normalizing neural networks[J]. Acta Physica Sinica, 2020, 69(6): 069701-1
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