Classification of Variable Stars Light Curves Using Long Short Term Memory Network

被引:5
|
作者
Bassi, Saksham [1 ]
Sharma, Kaushal [2 ]
Gomekar, Atharva [3 ]
机构
[1] NYU, Courant Inst Math Sci, New York, NY 10003 USA
[2] Aryabhatta Res Inst Observat Sci ARIES, Naini Tal, India
[3] Georgia Inst Technol, Atlanta, GA 30332 USA
关键词
deep learning; convolutional neural networks; long short term memory; variable star classification; big data and analytics; CONVOLUTIONAL NEURAL-NETWORKS; AUTOMATED SUPERVISED CLASSIFICATION; OGLE COLLECTION; MAGELLANIC-CLOUD; DISTANCE; CEPHEIDS; LSTM; GALAXY;
D O I
10.3389/fspas.2021.718139
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Owing to the current and upcoming extensive surveys studying the stellar variability, accurate and quicker methods are required for the astronomers to automate the classification of variable stars. The traditional approach of classification requires the calculation of the period of the observed light curve and assigning different variability patterns of phase folded light curves to different classes. However, applying these methods becomes difficult if the light curves are sparse or contain temporal gaps. Also, period finding algorithms start slowing down and become redundant in such scenarios. In this work, we present a new automated method, 1D CNN-LSTM, for classifying variable stars using a hybrid neural network of one-dimensional CNN and LSTM network which employs the raw time-series data from the variable stars. We apply the network to classify the time-series data obtained from the OGLE and the CRTS survey. We report the best average accuracy of 85% and F1 score of 0.71 for classifying five classes from the OGLE survey. We simultaneously apply other existing classification methods to our dataset and compare the results.
引用
收藏
页数:9
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