A Deep Learning Approach to Large-Scale Light Curve Prediction and Real-Time Anomaly Detection with Grubbs Criterion

Xiaodong Huang, Lei Peng, Cheng Lu, J. Bi, Haitao Yuan
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Abstract

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.
基于Grubbs准则的大规模光曲线预测和实时异常检测的深度学习方法
在光曲线(lc)中,恒星的亮度与时间有关,其图像也与时间有关。传统的数据处理方法不能有效地处理各种lc的实时、大容量数据。为了解决这个问题,这项工作开发了一个深度神经网络,名为基于dropout的递归神经网络(DRNN)。它通过长短期记忆单元,提取迷你陆基广角相机阵列(Mini- gwac)捕获的所有图像的复杂特征,进行点源提取和交叉认证。DRNN还可以对光变化曲线的异常值产生预警。此外,本文还对训练模型进行了优化,将dropout方法与自适应矩估计算法相结合,基于LCs数据迭代更新RNN的网络权重。在Mini-GWAC数据集上进行的大量实验表明,在大规模天文LCs中,DRNN在预测恒星亮度方面优于几种典型方法。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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