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Related papers: GRB 221009A, The BOAT

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Blazars and Gamma Ray Bursts (GRBs) are the fastest objects known so far. The radiation we see from these sources originates in a jet of similar aperture angle, and we think it is the result of the conversion of some of the jet kinetic…

Astrophysics · Physics 2011-07-19 G. Ghisellini

Identifying the astrophysical sites of the $r$-process, one of the primary mechanisms by which heavy elements are formed, is a key goal of modern astrophysics. The discovery of the brightest gamma-ray burst of all time, GRB 221009A, at a…

The brightest gamma ray burst (GRB) ever observed, GRB221009A, produced a surprisingly large flux of gamma rays with multi-TeV energies, which are expected to be absorbed in interactions with extragalactic background light (EBL). If the…

High Energy Astrophysical Phenomena · Physics 2025-06-16 Oleg Kalashev , Felix Aharonian , Warren Essey , Yoshiyuki Inoue , Alexander Kusenko

Gamma-ray bursts (GRBs) originate from explosions at cosmological distances, generating collimated jets. GRB 221009A, exploded on 9 October 2022, has been established as the brightest GRB to date. Its bright and long emission was…

High Energy Astrophysical Phenomena · Physics 2025-09-30 Arnau Aguasca-Cabot , Susumu Inoue , Monica Seglar-Arroyo , Kenta Terauchi , Pol Bordas , Marc Ribó

GRB 221009A was the brightest gamma-ray burst ever detected on Earth. In its early afterglow phase, photons with exceptional energies above 10 TeV were observed by LHAASO, and a photon-like air shower above 200 TeV was detected by Carpet-2.…

High Energy Astrophysical Phenomena · Physics 2024-01-12 Sergey Troitsky

The observations of the exceptionally bright gamma-ray burst (GRB) 130427A by the Large Area Telescope aboard the Fermi Gamma-ray Space Telescope provide constraints on the nature of such unique astrophysical sources. GRB 130427A had the…

High Energy Astrophysical Phenomena · Physics 2013-12-10 LAT collaboration , GBM collaboration

Long Gamma Ray Bursts are thought to originate from the core collapse of massive stars that give rise to energetic broad-lined Type Ic supernovae. The brightest burst ever recorded, GRB 221009A, has been linked to a broad-lined Type Ic…

High Energy Astrophysical Phenomena · Physics 2026-03-12 Rahim Moradi , Emre S. Yorgancioglu , Shao-Lin Xiong , Yan-Qiu Zhang , Shuang-Nan Zhang , Roland Diehl , Yu Wang

GRB221009A is the brightest gamma-ray burst ever detected. To probe the very-high-energy (VHE, $>$\!100 GeV) emission, the High Energy Stereoscopic System (H.E.S.S.) began observations 53 hours after the triggering event, when the…

High Energy Astrophysical Phenomena · Physics 2023-04-12 H. E. S. S. Collaboration , : , F. Aharonian , F. Ait Benkhali , J. Aschersleben , H. Ashkar , M. Backes , A. Baktash , V. Barbosa Martins , R. Batzofin , Y. Becherini , D. Berge , K. Bernlöhr , B. Bi , M. Böttcher , C. Boisson , J. Bolmont , M. de Bony de Lavergne , J. Borowska , M. Bouyahiaoui , F. Bradascio , M. Breuhaus , R. Brose , F. Brun , B. Bruno , T. Bulik , C. Burger-Scheidlin , S. Caroff , S. Casanova , J. Celic , M. Cerruti , T. Chand , S. Chandra , A. Chen , J. Chibueze , O. Chibueze , G. Cotter , S. Dai , J. Damascene Mbarubucyeye , J. Devin , A. Djannati-Ataï , A. Dmytriiev , V. Doroshenko , K. Egberts , S. Einecke , J. -P. Ernenwein , S. Fegan , G. Fichet de Clairfontaine , M. Filipovic , G. Fontaine , M. Füßling , S. Funk , S. Gabici , S. Ghafourizadeh , G. Giavitto , D. Glawion , J. F. Glicenstein , P. Goswami , G. Grolleron , M. -H. Grondin J. A. Hinton , T. L. Holch , M. Holler , D. Horns , Zhiqiu Huang , M. Jamrozy , F. Jankowsky , V. Joshi , I. Jung-Richardt , E. Kasai , K. Katarzyński , R. Khatoon , B. Khélifi , W. Kluźniak , Nu. Komin , R. Konno , K. Kosack , D. Kostunin , R. G. Lang , S. Le Stum , F. Leitl , A. Lemière , M. Lemoine-Goumard , J. P. Lenain , F. Leuschner , T. Lohse , I. Lypova , J. Mackey , D. Malyshev , D. Malyshev , V. Marandon , P. Marchegiani , A. Marcowith , G. Martí-Devesa , R. Marx , M. Meyer , A. Mitchell , L. Mohrmann , A. Montanari , E. Moulin , T. Murach , K. Nakashima , M. de Naurois , J. Niemiec , A. Priyana Noel , P. O'Brien , S. Ohm , L. Olivera-Nieto , E. de Ona Wilhelmi , M. Ostrowski , S. Panny , M. Panter , R. D. Parsons , G. Peron , D. A. Prokhorov , H. Prokoph , G. Pühlhofer , M. Punch , A. Quirrenbach , P. Reichherzer , A. Reimer , O. Reimer , H. Ren , M. Renaud , B. Reville , F. Rieger , G. Rowell , B. Rudak , E. Ruiz-Velasco , V. Sahakian , H. Salzmann , A. Santangelo , M. Sasaki , J. Schäfer , F. Schüssler , H. M. Schutte , U. Schwanke , J. N. S. Shapopi , A. Specovius , S. Spencer , Ł. Stawarz , R. Steenkamp , S. Steinmassl , C. Steppa , I. Sushch , H. Suzuki , T. Takahashi , T. Tanaka , R. Terrier , N. Tsuji , Y. Uchiyama , M. Vecchi , C. Venter , J. Vink , S. J. Wagner , R. White , A. Wierzcholska , Yu Wun Wong , M. Zacharias , D. Zargaryan , A. A. Zdziarski , A. Zech , S. J. Zhu , N. Żywucka

Gamma-ray burst (GRB) 130427A is one of the most energetic GRBs ever observed. The initial pulse up to 2.5 s is possibly the brightest well-isolated pulse observed to date. A fine time resolution spectral analysis shows power-law decays of…

High Energy Astrophysical Phenomena · Physics 2013-11-25 R. Preece , J. Michael Burgess , A. von Kienlin , P. N. Bhat , M. S. Briggs , D. Byrne , V. Chaplin , W. Cleveland , A. C. Collazzi , V. Connaughton , A. Diekmann , G. Fitzpatrick , S. Foley , M. Gibby , M. Giles , A. Goldstein , J. Greiner , D. Gruber , P. Jenke , R. M. Kippen , C. Kouveliotou , S. McBreen , C. Meegan , W. S. Paciesas , V. Pelassa , D. Tierney , A. J. van der Horst , C. Wilson-Hodge , S. Xiong , G. Younes , H. -F. Yu , M. Ackermann , M. Ajello , M. Axelsson , L. Baldini , G. Barbiellini , M. G. Baring , D. Bastieri , R. Bellazzini , E. Bissaldi , E. Bonamente , J. Bregeon , M. Brigida , P. Bruel , R. Buehler , S. Buson , G. A. Caliandro , R. A. Cameron , P. A. Caraveo , C. Cecchi , E. Charles , A. Chekhtman , J. Chiang , G. Chiaro , S. Ciprini , R. Claus , J. Cohen-Tanugi , L. R. Cominsky , J. Conrad , F. D'Ammando , A. de Angelis , F. de Palma , C. D. Dermer , R. Desiante , S. W. Digel , L. Di Venere , P. S. Drell , A. Drlica-Wagner , C. Favuzzi , A. Franckowiak , Y. Fukazawa , P. Fusco , F. Gargano , N. Gehrels , S. Germani , N. Giglietto , F. Giordano , M. Giroletti , G. Godfrey , J. Granot , I. A. Grenier , S. Guiriec , D. Hadasch , Y. Hanabata , A. K. Harding , M. Hayashida , S. Iyyani , T. Jogler , G. Jóannesson , T. Kawano , J. Knödlseder , D. Kocevski , M. Kuss , J. Lande , J. Larsson , S. Larsson , L. Latronico , F. Longo , F. Loparco , M. N. Lovellette , P. Lubrano , M. Mayer , M. N. Mazziotta , P. F. Michelson , T. Mizuno , M. E. Monzani , E. Moretti , A. Morselli , S. Murgia , R. Nemmen , E. Nuss , T. Nymark , M. Ohno , T. Ohsugi , A. Okumura , N. Omodei , M. Orienti , D. Paneque , J. S. Perkins , M. Pesce-Rollins , F. Piron , G. Pivato , T. A. Porter , J. L. Racusin , S. Rainò , R. Rando , M. Razzano , S. Razzaque , A. Reimer , O. Reimer , S. Ritz , M. Roth , F. Ryde , A. Sartori , J. D. Scargle , A. Schulz , C. Sgrò , E. J. Siskind , G. Spandre , P. Spinelli , D. J. Suson , H. Tajima , H. Takahashi , J. G. Thayer , J. B. Thayer , L. Tibaldo , M. Tinivella , D. F. Torres , G. Tosti , E. Troja , T. L. Usher , J. Vandenbroucke , V. Vasileiou , G. Vianello , V. Vitale , M. Werner , B. L. Winer , K. S. Wood , S. Zhu

As the brightest Gamma-Ray burst (GRB) ever detected, GRB 221009A may offer a chance that reveals some interesting features which are hidden in those bursts that are not so bright. There seems a very weak emission with a flux of…

High Energy Astrophysical Phenomena · Physics 2023-10-27 Xin-Ying Song , Shuang-Nan Zhang

With a redshift of z=6.295, GRB 050904 is the most distant gamma-ray burst ever discovered. It was an energetic event at all wavelengths and the afterglow was observed in detail in the near-infrared bands. We gathered all available optical…

Astrophysics · Physics 2008-11-26 D. A. Kann , N. Masetti , S. Klose

Gamma-ray bursts (GRB) are generally believed to be efficient particle accelerators. In the presence of energetic protons in a GRB jet, interactions between these protons and intense radiation field of the GRB are supposed to induce…

High Energy Astrophysical Phenomena · Physics 2023-02-01 Ruo-Yu Liu , Hai-Ming Zhang , Xiang-Yu Wang

Gamma-ray bursts (GRBs) are the most luminous electromagnetic explosions in the Universe, which emit up to $8.8\times10^{54}$ erg isotropic equivalent energy in the hard X-ray band. The high luminosity makes them detectable out to the…

High Energy Astrophysical Phenomena · Physics 2015-06-03 F. Y. Wang , Z. G. Dai , E. W. Liang

Recently an extraordinarily bright gamma-ray burst, GRB 221009A, was observed by several facilities covering the whole electromagnetic spectrum. Gamma rays with energies up to 18 TeV were detected, as well as a possible photon with 251 TeV.…

High Energy Astrophysical Phenomena · Physics 2022-12-27 Rafael Alves Batista

The two brightest and so far the best studied gamma ray bursts (GRBs), 990123 and 080319B, were ordinary, highly collimated GRBs produced in a core collapse supernova explosion within a high-density wind environment and observed from a very…

Astrophysics · Physics 2008-12-22 Shlomo Dado , Arnon Dar

About one month after the revolutionary discovery of the Gamma Ray Burst (GRB) GRB 221009A and intense theoretical efforts to explain its detection, time seems to us ripe to make an assessment of the axion-like particle (ALP) based…

High Energy Astrophysical Phenomena · Physics 2022-11-16 Giorgio Galanti , Marco Roncadelli , Fabrizio Tavecchio

GRB 221009A, the Brightest Of All Time (BOAT), presents a challenge for afterglow modelling due to its low Galactic latitude and consequent high line-of-sight extinction. This has led to a wide range of conflicting values for the optical…

On 9 October, 2022, an extremely powerful gamma-ray burst, GRB 221009A, was detected by several instruments. Despite being obstructed by the Milky Way galaxy, its afterglow outburst outshone all other GRBs seen before. LHAASO detected…

High Energy Astrophysical Phenomena · Physics 2023-01-18 Sarira Sahu , B. Medina-Carrillo , G. Sánchez-Colón , Subhash Rajpoot

The IceCube neutrino observatory detects the diffuse astrophysical neutrino background with high significance, but the contribution of different classes of sources is not established. Because of their non-thermal spectrum, gamma-ray bursts…

High Energy Astrophysical Phenomena · Physics 2024-08-30 P. Veres , N. Fraija , S. Lesage , A. Goldstein , M. S. Briggs , P. N. Bhat

GRB 980329 is the brightest gamma-ray burst detected so far with the Wide Field Cameras aboard BeppoSAX, both in gamma-rays and X-rays. With respect to its fluence (2.6 X 10**-5 erg/s/cm**2 in 50 to 300 keV) it would be in the top 4% of…