Machine learning search for variable stars
Ilya N. Pashchenko, Kirill V. Sokolovsky, Panagiotis Gavras

TL;DR
This paper introduces a machine learning approach to detect variable stars in photometric data, demonstrating improved efficiency over traditional methods by using classifiers like neural networks and ensemble algorithms.
Contribution
It proposes a novel variability detection method as a classification problem using machine learning, applicable to diverse variability types and robust to data issues.
Findings
Machine learning classifiers outperform traditional variability detection techniques.
Neural Networks, SGB, SVM, and RF show higher efficiency in identifying variable stars.
13 new low-amplitude variable stars discovered in the test set.
Abstract
Photometric variability detection is often considered as a hypothesis testing problem: an object is variable if the null-hypothesis that its brightness is constant can be ruled out given the measurements and their uncertainties. Uncorrected systematic errors limit the practical applicability of this approach to high-amplitude variability and well-behaving data sets. Searching for a new variability detection technique that would be applicable to a wide range of variability types while being robust to outliers and underestimated measurement uncertainties, we propose to consider variability detection as a classification problem that can be approached with machine learning. We compare several classification algorithms: Logistic Regression (LR), Support Vector Machines (SVM), k-Nearest Neighbors (kNN) Neural Nets (NN), Random Forests (RF) and Stochastic Gradient Boosting classifier (SGB)…
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