Morphological classification of eclipsing binary stars using computer vision methods
\v{S}tefan Parimucha, Maksim Gabdeev, Yanna Markus, Martin Va\v{n}ko, Pavol Gajdo\v{s}

TL;DR
This paper applies advanced computer vision techniques, including CNNs and vision transformers, to classify eclipsing binary star light curves with high accuracy, introducing a novel image representation to improve model generalization.
Contribution
The study develops a hierarchical classification approach using pre-trained models on synthetic data, achieving high accuracy in binary star classification and highlighting challenges in spot detection.
Findings
Binary classification accuracy exceeds 96% on validation data.
Models perform well (>94%) on observational data from multiple catalogs.
Spot detection accuracy remains low, indicating a need for further research.
Abstract
We present an application of computer vision methods to classify the light curves of eclipsing binaries (EB). We have used pre-trained models based on convolutional neural networks () and vision transformers (), which were fine-tuned on images created from synthetic datasets. To improve model generalisation and reduce overfitting, we developed a novel image representation by transforming phase-folded light curves into polar coordinates combined with hexbin visualisation. Our hierarchical approach in the first stage classifies systems into detached and overcontact types, and in the second stage identifies the presence or absence of spots. The binary classification models achieved high accuracy () on validation data across multiple passbands (Gaia~, , and ) and demonstrated strong performance (, up to …
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Taxonomy
TopicsStellar, planetary, and galactic studies · Astronomy and Astrophysical Research · History and Developments in Astronomy
