Estimating the peak energy of Swift gamma-ray bursts using supervised machine learning
Gamma-ray bursts (GRBs) are among the most energetic explosive phenomena in the Universe, and their peak energy (Ep) is a key physical quantity for understanding the prompt emission mechanism. However, due to the limited energy coverage of the Swift satellite, a large fraction of Swift GRBs lack rel...
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| Hauptverfasser: | , , , |
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| Format: | Artigo |
| Sprache: | Inglês |
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EDP Sciences
2026-04-01
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| Schriftenreihe: | Astronomy & Astrophysics |
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| Online-Zugang: | https://www.aanda.org/articles/aa/full_html/2026/04/aa58857-26/aa58857-26.html |
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