Image-based Classification of Variable Stars: First Results from Optical Gravitational Lensing Experiment Data

ASTROPHYSICAL JOURNAL LETTERS(2020)

Cited 11|Views18
No score
Abstract
Recently, machine learning methods have presented a viable solution for the automated classification of image-based data in various research fields and business applications. Scientists require a fast and reliable solution in order to handle increasingly large amounts of astronomical data. However, so far astronomers have been mainly classifying variable starlight curves based on various pre-computed statistics and light curve parameters. In this work we use an image-based Convolutional Neural Network to classify the different types of variable stars. We use images of phase-folded light curves from the Optical Gravitational Lensing Experiment (OGLE)-III survey for training, validating, and testing, and use OGLE-IV survey as an independent data set for testing. After the training phase, our neural network was able to classify the different types between 80% and 99%, and 77%-98%, accuracy for OGLE-III and OGLE-IV, respectively.
More
Translated text
Key words
Astronomy data analysis,Anomalous Cepheid variable stars,Eclipsing binary stars,Delta Scuti variable stars,RR Lyrae variable stars,Periodic variable stars,Type II Cepheid variable stars,Convolutional neural networks,Sky surveys,Classification,Light curve classification
AI Read Science
Must-Reading Tree
Example
Generate MRT to find the research sequence of this paper
Chat Paper
Summary is being generated by the instructions you defined