Axelsson M, Ajello M, Arimoto M, Baldini L, Ballet J, Baring MG, Bartolini C, Bastieri D, Becerra Gonzalez J, Bellazzini R, Berenji B, Bissaldi E, Blandford RD, Bonino R, Bruel P, Buson S, Cameron RA, Caputo R, Caraveo PA, Cavazzuti E, Cheung CC, Chiaro G, Cibrario N, Ciprini S, Cozzolongo G, Cristarella Orestano P, Crnogorcevic M, Cuoco A, Cutini S, D’Ammando F, De Gaetano S, Di Lalla N, Dinesh A, Di Tria R, Di Venere L, Domínguez A, Fegan SJ, Ferrara EC, Fiori A, Franckowiak A, Fukazawa Y, Funk S, Fusco P, Galanti G, Gargano F, Gasbarra C, Germani S, Giacchino F, Giglietto N, Giliberti M, Gill R, Giordano F, Giroletti M, Granot J, Green D, Grenier IA, Guiriec S, Gustafsson M, Hashizume M, Hays E, Hewitt JW, Horan D, Kayanoki T, Kuss M, Laviron A, Li J, Liodakis I, Longo F, Loparco F, Lorusso L, Lott B, Lovellette MN, Lubrano P, Maldera S, Malyshev D, Manfreda A, Martí-Devesa G, Martinelli R, Martinez Castellanos I, Mazziotta MN, McEnery JE, Mereu I, Meyer M, Michelson PF, Mirabal N, Mitthumsiri W, Mizuno T, Monti-Guarnieri P, Monzani ME, Morishita T, Morselli A, Moskalenko IV, Negro M, Niwa R, Omodei N, Orienti M, Orlando E, Paneque D, Panzarini G, Persic M, Pesce-Rollins M, Petrosian V, Pillera R, Piron F, Porter TA, Principe G, Racusin JL, Rainò S, Rando R, Rani B, Razzano M, Razzaque S, Reimer A, Reimer O, Ryde F, Sánchez-Conde M, Saz Parkinson PM, Serini D, Sgrò C, Sharma V, Siskind EJ, Spandre G, Spinelli P, Suson DJ, Tajima H, Tak D, Thayer JB, Torres DF, Valverde J, Zaharijas G, Lesage S, Briggs MS, Burns E, Bala S, Bhat PN, Cleveland WH, Dalessi S, de Barra C, Gibby M, Giles MM, Hamburg R, Hristov BA, Kocevski D, Hui CM, Mailyan B, Malacaria C, McBreen S, Poolakkil S, Roberts OJ, Scotton L, Veres P, von Kienlin A, Wilson-Hodge CA, Wood J (2025)
Publication Type: Journal article
Publication year: 2025
Book Volume: 277
Article Number: 24
Journal Issue: 1
We present a complete analysis of Fermi Large Area Telescope (LAT) data of GRB 221009A, the brightest gamma-ray burst (GRB) ever detected. The burst emission above 30 MeV detected by the LAT preceded, by 1 s, the low-energy (<10 MeV) pulse that triggered the Fermi Gamma-Ray Burst Monitor (GBM), as has been observed in other GRBs. The prompt phase of GRB 221009A lasted a few hundred seconds. It was so bright that we identify a bad time interval of 64 s caused by the extremely high flux of hard X-rays and soft gamma rays, during which the event reconstruction efficiency was poor and the dead time fraction quite high. The late-time emission decayed as a power law, but the extrapolation of the late-time emission during the first 450 s suggests that the afterglow started during the prompt emission. We also found that high-energy events observed by the LAT are incompatible with synchrotron origin, and, during the prompt emission, are more likely related to an extra component identified as synchrotron self-Compton (SSC). A remarkable 400 GeV photon, detected by the LAT 33 ks after the GBM trigger and directionally consistent with the location of GRB 221009A, is hard to explain as a product of SSC or TeV electromagnetic cascades, and the process responsible for its origin is uncertain. Because of its proximity and energetic nature, GRB 221009A is an extremely rare event.
APA:
Axelsson, M., Ajello, M., Arimoto, M., Baldini, L., Ballet, J., Baring, M.G.,... Wood, J. (2025). GRB 221009A: The B.O.A.T. Burst that Shines in Gamma Rays. Astrophysical Journal Supplement Series, 277(1). https://doi.org/10.3847/1538-4365/ada272
MLA:
Axelsson, M., et al. "GRB 221009A: The B.O.A.T. Burst that Shines in Gamma Rays." Astrophysical Journal Supplement Series 277.1 (2025).
BibTeX: Download