TY - GEN
T1 - A Deep Learning Approach to Large-Scale Light Curve Prediction and Real-Time Anomaly Detection with Grubbs Criterion
AU - Huang, Xiaodong
AU - Peng, Lei
AU - Lu, Cheng
AU - Bi, Jing
AU - Yuan, Haitao
N1 - Publisher Copyright:
© 2020 IEEE.
PY - 2020/10/30
Y1 - 2020/10/30
N2 - In light curves (LCs), the brightness of stars is associated with time, and so is its image. The traditional data processing methods cannot effectively handle real-time and large-volume data of various LCs. To address this issue, this work develops a deep neural network named Dropout-based Recurrent Neural Networks (DRNN). It extracts complicated features of all images captured by Mini Ground-based Wide-Angle Camera array (Mini-GWAC) for point source extraction and cross-certification through Long Short-Term Memory units. DRNN can also produce warnings for abnormal values of light change curves. Furthermore, this work optimizes the training model by combining a dropout method with an adaptive moment estimation algorithm to iteratively update the network weight of the RNN based on the LCs data. Extensive experiments with a Mini-GWAC dataset demonstrate that DRNN outperforms several typical methods in terms of prediction performance of star brightness in large-scale astronomical LCs.
AB - In light curves (LCs), the brightness of stars is associated with time, and so is its image. The traditional data processing methods cannot effectively handle real-time and large-volume data of various LCs. To address this issue, this work develops a deep neural network named Dropout-based Recurrent Neural Networks (DRNN). It extracts complicated features of all images captured by Mini Ground-based Wide-Angle Camera array (Mini-GWAC) for point source extraction and cross-certification through Long Short-Term Memory units. DRNN can also produce warnings for abnormal values of light change curves. Furthermore, this work optimizes the training model by combining a dropout method with an adaptive moment estimation algorithm to iteratively update the network weight of the RNN based on the LCs data. Extensive experiments with a Mini-GWAC dataset demonstrate that DRNN outperforms several typical methods in terms of prediction performance of star brightness in large-scale astronomical LCs.
KW - Light curves
KW - anomaly detection optimization
KW - dropout
KW - recurrent neural networks
KW - time series prediction
UR - https://www.scopus.com/pages/publications/85096351662
U2 - 10.1109/ICNSC48988.2020.9238105
DO - 10.1109/ICNSC48988.2020.9238105
M3 - 会议稿件
AN - SCOPUS:85096351662
T3 - 2020 IEEE International Conference on Networking, Sensing and Control, ICNSC 2020
BT - 2020 IEEE International Conference on Networking, Sensing and Control, ICNSC 2020
PB - Institute of Electrical and Electronics Engineers Inc.
T2 - 2020 IEEE International Conference on Networking, Sensing and Control, ICNSC 2020
Y2 - 30 October 2020 through 2 November 2020
ER -