Image-based Classification of Variable Stars: First Results from Optical Gravitational Lensing Experiment Data
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.
- Publication:
-
The Astrophysical Journal
- Pub Date:
- July 2020
- DOI:
- arXiv:
- arXiv:2006.07614
- Bibcode:
- 2020ApJ...897L..12S
- Keywords:
-
- RR Lyrae variable stars;
- Classification;
- Light curve classification;
- Astronomy data analysis;
- Type II Cepheid variable stars;
- Anomalous Cepheid variable stars;
- Delta Scuti variable stars;
- Eclipsing binary stars;
- Periodic variable stars;
- Convolutional neural networks;
- Sky surveys;
- 1410;
- 1907;
- 1954;
- 1858;
- 2124;
- 2106;
- 370;
- 444;
- 1213;
- 1938;
- 1464;
- Astrophysics - Solar and Stellar Astrophysics;
- Astrophysics - Instrumentation and Methods for Astrophysics
- E-Print:
- Accepted in ApJL, 11pages, 5 figures, 8 tables