Automated supervised classification of variable stars II. Application to the OGLE database

TL;DR

This paper develops and tests an automated classification system for variable stars, applying it to the OGLE database to identify and analyze different variability classes, including B-stars, with a focus on reliability and new class identification.

Contribution

The study extends previous classifiers, incorporates color information, and demonstrates a fast, reliable system for classifying large-scale variable star data in the OGLE survey.

Findings

The classifier accurately identifies main variability classes.

It reveals new samples of variable stars in OGLE data.

The system efficiently processes large datasets.

Abstract

We aim to extend and test the classifiers presented in a previous work against an independent dataset. We complement the assessment of the validity of the classifiers by applying them to the set of OGLE light curves treated as variable objects of unknown class. The results are compared to published classification results based on the so-called extractor methods.Two complementary analyses are carried out in parallel. In both cases, the original time series of OGLE observations of the Galactic bulge and Magellanic Clouds are processed in order to identify and characterize the frequency components. In the first approach, the classifiers are applied to the data and the results analyzed in terms of systematic errors and differences between the definition samples in the training set and in the extractor rules. In the second approach, the original classifiers are extended with colour information and, again, applied to OGLE light curves. We have constructed a classification system that can process huge amounts of time series in negligible time and provide reliable samples of the main variability classes. We have evaluated its strengths and weaknesses and provide potential users of the classifier with a detailed description of its characteristics to aid in the interpretation of classification results. Finally, we apply the classifiers to obtain object samples of classes not previously studied in the OGLE database and analyse the results. We pay specific attention to the B-stars in the samples, as their pulsations are strongly dependent on metallicity.