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...
I tiakina i:
| Ngā kaituhi matua: | , , , |
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| Hōputu: | Artigo |
| Reo: | Inglês |
| I whakaputaina: |
EDP Sciences
2026-04-01
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| Rangatū: | Astronomy & Astrophysics |
| Ngā marau: | |
| Urunga tuihono: | https://www.aanda.org/articles/aa/full_html/2026/04/aa58857-26/aa58857-26.html |
| Ngā Tūtohu: |
Kāore He Tūtohu, Me noho koe te mea tuatahi ki te tūtohu i tēnei pūkete!
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