ASTRAFier: A Novel and Scalable Transformer-based Stellar Variability Classifier
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arXiv
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| Autori principali: | , , , , , , , |
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| Natura: | Preprint |
| Pubblicazione: |
2026
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| _version_ | 1866911578723450880 |
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| author | Gregory, Paul F. X. Audenaert, Jeroen Kliapets, Mykyta Muthukrishna, Daniel Tkachenko, Andrew Skarka, Marek Hon, Marc Ricker, George R. |
| author_facet | Gregory, Paul F. X. Audenaert, Jeroen Kliapets, Mykyta Muthukrishna, Daniel Tkachenko, Andrew Skarka, Marek Hon, Marc Ricker, George R. |
| contents | Photometric missions such as Kepler and TESS have generated millions of light curves covering almost the entire sky, offering unprecedented opportunities to study stellar variability and advance our understanding of the Universe. In this data-rich environment, machine learning has emerged as a powerful tool to efficiently and accurately process and classify light curves according to their type of stellar variability. In this work, we introduce ASTRAFier: a novel Transformer-based model for variability classification that integrates Bidirectional Long Short-Term Memory (BiLSTM) and Convolutional Neural Networks (CNNs). The model operates directly on time series without requiring feature engineering, creating an easy-to-maintain and efficient end-to-end classification framework. We train and validate our model using both Kepler and TESS light curves and, respectively, achieve a classification accuracy of $94.26\%$ on Kepler and $88.22\%$ on TESS. We demonstrate scalability by deploying our model on $\sim 2.8$ million TESS light curves from sectors 14, 15, and 26 (Kepler Field-of-View) delivered by MIT's Quick-look Pipeline (QLP) and release the resulting stellar variability catalog. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2604_07437 |
| institution | arXiv |
| publishDate | 2026 |
| record_format | arxiv |
| spellingShingle | ASTRAFier: A Novel and Scalable Transformer-based Stellar Variability Classifier Gregory, Paul F. X. Audenaert, Jeroen Kliapets, Mykyta Muthukrishna, Daniel Tkachenko, Andrew Skarka, Marek Hon, Marc Ricker, George R. Instrumentation and Methods for Astrophysics Solar and Stellar Astrophysics Photometric missions such as Kepler and TESS have generated millions of light curves covering almost the entire sky, offering unprecedented opportunities to study stellar variability and advance our understanding of the Universe. In this data-rich environment, machine learning has emerged as a powerful tool to efficiently and accurately process and classify light curves according to their type of stellar variability. In this work, we introduce ASTRAFier: a novel Transformer-based model for variability classification that integrates Bidirectional Long Short-Term Memory (BiLSTM) and Convolutional Neural Networks (CNNs). The model operates directly on time series without requiring feature engineering, creating an easy-to-maintain and efficient end-to-end classification framework. We train and validate our model using both Kepler and TESS light curves and, respectively, achieve a classification accuracy of $94.26\%$ on Kepler and $88.22\%$ on TESS. We demonstrate scalability by deploying our model on $\sim 2.8$ million TESS light curves from sectors 14, 15, and 26 (Kepler Field-of-View) delivered by MIT's Quick-look Pipeline (QLP) and release the resulting stellar variability catalog. |
| title | ASTRAFier: A Novel and Scalable Transformer-based Stellar Variability Classifier |
| topic | Instrumentation and Methods for Astrophysics Solar and Stellar Astrophysics |
| url | https://arxiv.org/abs/2604.07437 |