Repeating versus Nonrepeating Fast Radio Bursts: A Deep Learning Approach to Morphological Characterization
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arXiv
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| Autori principali: | , , , , , , , , |
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| Natura: | Preprint |
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2025
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| _version_ | 1866910015035539456 |
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| author | Kharel, Bikash Fonseca, Emmanuel Brar, Charanjot Khan, Afrokk Mas-Ribas, Lluis Patil, Swarali Shivraj Scholz, Paul Siegel, Seth Robert Stenning, David C. |
| author_facet | Kharel, Bikash Fonseca, Emmanuel Brar, Charanjot Khan, Afrokk Mas-Ribas, Lluis Patil, Swarali Shivraj Scholz, Paul Siegel, Seth Robert Stenning, David C. |
| contents | We present a deep learning approach to classify fast radio bursts (FRBs) based purely on morphology as encoded on recorded dynamic spectrum from CHIME/FRB Catalog 2. We implemented transfer learning with a pretrained ConvNext architecture, exploiting its powerful feature extraction ability. ConvNext was adapted to classify dedispersed dynamic spectra (which we treat as images) of the FRBs into one of the two sub-classes, i.e., repeater and non-repeater, based on their various temporal and spectral properties and relation between the sub-pulse structures. Additionally, we also used mathematical model representation of the total intensity data to interpret the deep learning model. Upon fine-tuning the pretrained ConvNext on the FRB spectrograms, we were able to achieve high classification metrics while substantially reducing training time and computing power as compared to training a deep learning model from scratch with random weights and biases without any feature extraction ability. Importantly, our results suggest that the morphological differences between CHIME repeating and non-repeating events persist in Catalog 2 and the deep learning model leveraged these differences for classification. The fine-tuned deep learning model can be used for inference, which enables us to predict whether an FRB's morphology resembles that of repeaters or non-repeaters. Such inferences may become increasingly significant when trained on larger data sets that will exist in the near future. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2509_06208 |
| institution | arXiv |
| publishDate | 2025 |
| record_format | arxiv |
| spellingShingle | Repeating versus Nonrepeating Fast Radio Bursts: A Deep Learning Approach to Morphological Characterization Kharel, Bikash Fonseca, Emmanuel Brar, Charanjot Khan, Afrokk Mas-Ribas, Lluis Patil, Swarali Shivraj Scholz, Paul Siegel, Seth Robert Stenning, David C. High Energy Astrophysical Phenomena Machine Learning We present a deep learning approach to classify fast radio bursts (FRBs) based purely on morphology as encoded on recorded dynamic spectrum from CHIME/FRB Catalog 2. We implemented transfer learning with a pretrained ConvNext architecture, exploiting its powerful feature extraction ability. ConvNext was adapted to classify dedispersed dynamic spectra (which we treat as images) of the FRBs into one of the two sub-classes, i.e., repeater and non-repeater, based on their various temporal and spectral properties and relation between the sub-pulse structures. Additionally, we also used mathematical model representation of the total intensity data to interpret the deep learning model. Upon fine-tuning the pretrained ConvNext on the FRB spectrograms, we were able to achieve high classification metrics while substantially reducing training time and computing power as compared to training a deep learning model from scratch with random weights and biases without any feature extraction ability. Importantly, our results suggest that the morphological differences between CHIME repeating and non-repeating events persist in Catalog 2 and the deep learning model leveraged these differences for classification. The fine-tuned deep learning model can be used for inference, which enables us to predict whether an FRB's morphology resembles that of repeaters or non-repeaters. Such inferences may become increasingly significant when trained on larger data sets that will exist in the near future. |
| title | Repeating versus Nonrepeating Fast Radio Bursts: A Deep Learning Approach to Morphological Characterization |
| topic | High Energy Astrophysical Phenomena Machine Learning |
| url | https://arxiv.org/abs/2509.06208 |