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Related papers: The Multiwavelength Picture of GRB 221009A's After…

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Gamma-ray bursts (GRBs) are the most energetic explosions in the universe, and their afterglow emission provides an opportunity to probe the physics of relativistic shock waves in an extreme environment. Several key pieces for completing…

The early afterglow of a Gamma-ray burst (GRB) can provide critical information on the jet and progenitor of the GRB. The extreme brightness of GRB 221009A allows us to probe its early afterglow in unprecedented detail. In this letter, we…

Observations of long duration gamma-ray bursts (GRBs) with TeV emission during their afterglow have been on the rise. Recently, GRB 221009A, the most energetic GRB ever observed, was detected by the {LHAASO} experiment in the energy band…

High Energy Astrophysical Phenomena · Physics 2023-08-15 Hebzibha Isravel , Damien Begue , Asaf Pe'er

GRB 221009A ($z=0.151$) is one of the closest known long $\gamma$-ray bursts (GRBs). Its extreme brightness across all electromagnetic wavelengths provides an unprecedented opportunity to study a member of this still-mysterious class of…

Some gamma-ray bursts (GRBs) have an afterglow in the tera-electronvolt (TeV) band, but the early onset of this afterglow has not been observed. We report observations with the Large High Altitude Air Shower Observatory of the bright GRB…

High Energy Astrophysical Phenomena · Physics 2023-07-11 LHAASO Collaboration

We study GRB 221009A, the brightest gamma-ray burst in the history of observations, using Fermi data. To calibrate them for large inclination angles, we use the Vela X gamma-ray source. Light curves in different spectral ranges demonstrate…

High Energy Astrophysical Phenomena · Physics 2023-03-22 B. Stern , I. Tkachev

GRB 221009A is the brightest gamma-ray burst ever detected since the discovery of this kind of energetic explosions. However, an accurate measurement of the prompt emission properties of this burst is very challenging due to its exceptional…

High Energy Astrophysical Phenomena · Physics 2023-03-06 Zheng-Hua An , S. Antier , Xing-Zi Bi , Qing-Cui Bu , Ce Cai , Xue-Lei Cao , Anna-Elisa Camisasca , Zhi Chang , Gang Chen , Li Chen , Tian-Xiang Chen , Wen Chen , Yi-Bao Chen , Yong Chen , Yu-Peng Chen , Michael W. Coughlin , Wei-Wei Cui , Zi-Gao Dai , T. Hussenot-Desenonges , Yan-Qi Du , Yuan-Yuan Du , Yun-Fei Du , Cheng-Cheng Fan , Filippo Frontera , He Gao , Min Gao , Ming-Yu Ge , Ke Gong , Yu-Dong Gu , Ju Guan , Dong-Ya Guo , Zhi-Wei Guo , Cristiano Guidorzi , Da-Wei Han , Jian-Jian He , Jun-Wang He , Dong-Jie Hou , Yue Huang , Jia Huo , Zhen Ji , Shu-Mei Jia , Wei-Chun Jiang , David Alexander Kann , A. Klotz , Ling-Da Kong , Lin Lan , An Li , Bing Li , Chao-Yang Li , Cheng-Kui Li , Gang Li , Mao-Shun Li , Ti-Pei Li , Wei Li , Xiao-Bo Li , Xin-Qiao Li , Xu-Fang Li , Yan-Guo Li , Zheng-Wei Li , Jing Liang , Xiao-Hua Liang , Jin-Yuan Liao , Lin Lin , Cong-Zhan Liu , He-Xin Liu , Hong-Wei Liu , Jia-Cong Liu , Xiao-Jing Liu , Ya-Qing Liu , Yu-Rong Liu , Fang-Jun Lu , Hong Lu , Xue-Feng Lu , Qi Luo , Tao Luo , Bin-Yuan Ma , Fu-Li Ma , Rui-Can Ma , Xiang Ma , Romain Maccary , Ji-Rong Mao , Bin Meng , Jian-Yin Nie , Mauro Orlandini , Ge Ou , Jing-Qiang Peng , Wen-Xi Peng , Rui Qiao , Jin-Lu Qu , Xiao-Qin Ren , Jing-Yan Shi , Qi Shi , Li-Ming Song , Xin-Ying Song , Ju Su , Gong-Xing Sun , Liang Sun , Xi-Lei Sun , Wen-Jun Tan , Ying Tan , Lian Tao , You-Li Tuo , Damien Turpin , Jin-Zhou Wang , Chen Wang , Chen-Wei Wang , Hong-Jun Wang , Hui Wang , Jin Wang , Ling-Jun Wang , Peng-Ju Wang , Ping Wang , Wen-Shuai Wang , Xiang-Yu Wang , Xi-Lu Wang , Yu-Sa Wang , Yue Wang , Xiang-Yang Wen , Bo-Bing Wu , Bai-Yang Wu , Hong Wu , Sheng-Hui Xiao , Shuo Xiao , Yun-Xiang Xiao , Sheng-Lun Xie , Shao-Lin Xiong , Sen-Lin Xiong , Dong Xu , He Xu , Yan-Jun Xu , Yan-Bing Xu , Ying-Chen Xu , Yu-Peng Xu , Wang-Chen Xue , Sheng Yang , Yan-Ji Yang , Zi-Xu Yang , Wen-Tao Ye , Qi-Bin Yi , Shu-Xu Yi , Qian-Qing Yin , Yuan You , Yun-Wei Yu , Wei Yu , Wen-Hui Yu , Ming Zeng , Bing Zhang , Bin-Bin Zhang , Da-Li Zhang , Fan Zhang , Hong-Mei Zhang , Juan Zhang , Liang Zhang , Peng Zhang , Peng Zhang , Shu Zhang , Shuang-Nan Zhang , Wan-Chang Zhang , Xiao-Feng Zhang , Xiao-Lu Zhang , Yan-Qiu Zhang , Yan-Ting Zhang , Yi-Fei Zhang , Yuan-Hang Zhang , Zhen Zhang , Guo-Ying Zhao , Hai-Sheng Zhao , Hong-Yu Zhao , Qing-Xia Zhao , Shu-Jie Zhao , Xiao-Yun Zhao , Xiao-Fan Zhao , Yi Zhao , Chao Zheng , Shi-Jie Zheng , Deng-Ke Zhou , Xing Zhou , Xiao-Cheng Zhu

GRB~221009A has been the brightest gamma-ray burst (GRB) observed to date, and its afterglow has been characterised with unprecedented detail at TeV energies by LHAASO. Quite puzzlingly, it is also the most energetic GRB known. Among the…

High Energy Astrophysical Phenomena · Physics 2026-01-21 O. S. Salafia , A. Celotti , E. Sobacchi , L. Nava , G. Oganesyan , G. Ghirlanda , S. Boula , M. E. Ravasio , G. Ghisellini

The highly variable and energetic pulsed emission of a long gamma-ray burst (GRB) is thought to originate from local, rapid dissipation of kinetic or magnetic energy within an ultra-relativistic jet launched by a newborn compact object,…

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 extraordinary gamma-ray burst GRB 221009A provides a great opportunity to investigate the enigmatic origin and evolution of GRBs. However, the complexity of the observations associated with this GRB provides significant challenges to…

High Energy Astrophysical Phenomena · Physics 2024-09-26 L. Foffano , M. Tavani , G. Piano

GRB 221009A was the Brightest gamma-ray burst Of All Time (BOAT), surpassing in prompt brightness all GRBs discovered in ~50 yr and in afterglow brightness in ~20 yr. We observed the BOAT with XMM-Newton 2.3 d after the prompt. The X-ray…

High Energy Astrophysical Phenomena · Physics 2024-08-07 Sergio Campana , Valentina Braito , Davide Lazzati , Andrea Tiengo

Gamma-ray burst (GRB), GRB 221009A, a long-duration GRB, was observed simultaneously by the Water Cherenkov Detector Array (WCDA) and the Kilometer Squared Array (KM2A) of the Large High Altitude Air Shower Observatory (LHAASO) during the…

High Energy Astrophysical Phenomena · Physics 2024-07-08 Sarira Sahu , B. Medina-Carrillo , D. I. Páez-Sánchez , G. Sánchez-Colón , Subhash Rajpoot

The highest energy gamma-rays from gamma-ray bursts (GRBs) have important implications for their radiation mechanism. Here we report for the first time the detection of gamma-rays up to 13 TeV from the brightest GRB 221009A by the Large…

High Energy Astrophysical Phenomena · Physics 2023-11-27 Zhen Cao , F. Aharonian , Q. An , A. Axikegu , Y. X. Bai , Y. W. Bao , D. Bastieri , X. J. Bi , Y. J. Bi , J. T. Cai , Q. Cao , W. Y. Cao , Zhe Cao , J. Chang , J. F. Chang , A. M. Chen , E. S. Chen , Liang Chen , Lin Chen , Long Chen , M. J. Chen , M. L. Chen , Q. H. Chen , S. H. Chen , S. Z. Chen , T. L. Chen , Y. Chen , N. Cheng , Y. D. Cheng , M. Y. Cui , S. W. Cui , X. H. Cui , Y. D. Cui , B. Z. Dai , H. L. Dai , Z. G. Dai , Danzengluobu , D. della Volpe , X. Q. Dong , K. K. Duan , J. H. Fan , Y. Z. Fan , J. Fang , K. Fang , C. F. Feng , L. Feng , S. H. Feng , X. T. Feng , Y. L. Feng , S. Gabici , B. Gao , C. D. Gao , L. Q. Gao , Q. Gao , W. Gao , W. K. Gao , M. M. Ge , L. S. Geng , G. Giacinti , G. H. Gong , Q. B. Gou , M. H. Gu , F. L. Guo , X. L. Guo , Y. Q. Guo , Y. Y. Guo , Y. A. Han , H. H. He , H. N. He , J. Y. He , X. B. He , Y. He , M. Heller , Y. K. Hor , B. W. Hou , C. Hou , X. Hou , H. B. Hu , Q. Hu , S. C. Hu , D. H. Huang , T. Q. Huang , W. J. Huang , X. T. Huang , X. Y. Huang , Y. Huang , Z. C. Huang , X. L. Ji , H. Y. Jia , K. Jia , K. Jiang , X. W. Jiang , Z. J. Jiang , M. Jin , M. M. Kang , T. Ke , D. Kuleshov , K. Kurinov , B. B. Li , Cheng Li , Cong Li , D. Li , F. Li , H. B. Li , H. C. Li , H. Y. Li , J. Li , Jian Li , Jie Li , K. Li , W. L. Li , W. L. Li , X. R. Li , Xin Li , Y. Z. Li , Zhe Li , Zhuo Li , E. W. Liang , Y. F. Liang , S. J. Lin , B. Liu , C. Liu , D. Liu , H. Liu , H. D. Liu , J. Liu , J. L. Liu , J. Y. Liu , M. Y. Liu , R. Y. Liu , S. M. Liu , W. Liu , Y. Liu , Y. N. Liu , R. Lu , Q. Luo , H. K. Lv , B. Q. Ma , L. L. Ma , X. H. Ma , J. R. Mao , Z. Min , W. Mitthumsiri , H. J. Mu , Y. C. Nan , A. Neronov , Z. W. Ou , B. Y. Pang , P. Pattarakijwanich , Z. Y. Pei , M. Y. Qi , Y. Q. Qi , B. Q. Qiao , J. J. Qin , D. Ruffolo , A. Sáiz , D. Semikoz , C. Y. Shao , L. Shao , O. Shchegolev , X. D. Sheng , F. W. Shu , H. C. Song , Yu. V. Stenkin , V. Stepanov , Y. Su , Q. N. Sun , X. N. Sun , Z. B. Sun , P. H. T. Tam , Q. W. Tang , Z. B. Tang , W. W. Tian , C. Wang , C. B. Wang , G. W. Wang , H. G. Wang , H. H. Wang , J. C. Wang , K. Wang , L. P. Wang , L. Y. Wang , P. H. Wang , R. Wang , W. Wang , X. G. Wang , X. Y. Wang , Y. Wang , Y. D. Wang , Y. J. Wang , Z. H. Wang , Z. X. Wang , Zhen Wang , Zheng Wang , D. M. Wei , J. J. Wei , Y. J. Wei , T. Wen , C. Y. Wu , H. R. Wu , S. Wu , X. F. Wu , Y. S. Wu , S. Q. Xi , J. Xia , J. J. Xia , G. M. Xiang , D. X. Xiao , G. Xiao , G. G. Xin , Y. L. Xin , Y. Xing , Z. Xiong , D. L. Xu , R. F. Xu , R. X. Xu , W. L. Xu , L. Xue , D. H. Yan , J. Z. Yan , T. Yan , C. W. Yang , F. Yang , F. F. Yang , H. W. Yang , J. Y. Yang , L. L. Yang , M. J. Yang , R. Z. Yang , S. B. Yang , Y. H. Yao , Z. G. Yao , Y. M. Ye , L. Q. Yin , N. Yin , X. H. You , Z. Y. You , Y. H. Yu , Q. Yuan , H. Yue , H. D. Zeng , T. X. Zeng , W. Zeng , M. Zha , B. B. Zhang , F. Zhang , H. M. Zhang , H. Y. Zhang , J. L. Zhang , L. X. Zhang , Li Zhang , P. F. Zhang , P. P. Zhang , R. Zhang , S. B. Zhang , S. R. Zhang , S. S. Zhang , X. Zhang , X. P. Zhang , Y. F. Zhang , Yi Zhang , Yong Zhang , B. Zhao , J. Zhao , L. Zhao , L. Z. Zhao , S. P. Zhao , F. Zheng , B. Zhou , H. Zhou , J. N. Zhou , M. Zhou , P. Zhou , R. Zhou , X. X. Zhou , C. G. Zhu , F. R. Zhu , H. Zhu , K. J. Zhu , X. Zuo

Flares are usually observed during the afterglow phase of Gamma-Ray Bursts (GRBs) in soft X-ray, optical and radio bands, but rarely in gamma-ray band. Despite the extraordinary brightness, GECAM-C has accurately measured both the bright…

The detection of $\gamma$-ray candidates up to the energy of $\approx$13 TeV from the exceptionally bright $\gamma$-ray burst GRB 221009A by the Large High Altitude Air-Shower Observatory (LHAASO) has raised considerable interest in the…

High Energy Astrophysical Phenomena · Physics 2026-04-14 Timur A. Dzhatdoev , Jagdish C. Joshi , Abhijit Roy , Grigory I. Rubtsov , Anatoly A. Semenov

X-ray light curves of gamma-ray burst (GRB) afterglows exhibit various features, with the shallow decay phase being particularly puzzling. While some studies report absence of the X-ray shallow decay for hyper-energetic GRBs, recently…

High Energy Astrophysical Phenomena · Physics 2025-04-16 Kenta Terauchi , Tomohiko Oka , Katsuaki Asano

The detection of gamma-ray burst GRB~221009A has attracted significant attention due to its record brightness and the first-ever detection of multi-TeV $\gamma$-rays from a GRB. Located at redshift $z=0.151$, this event is relatively nearby…

High Energy Astrophysical Phenomena · Physics 2025-08-14 Hassan Abdalla

Acceleration of hadrons in relativistic shocks has been long expected and invoked to model GRB high-energy photon and neutrino emissions. However, so far there has been no direct observational evidence of hadronic emission from GRBs. The…

High Energy Astrophysical Phenomena · Physics 2023-10-19 Kai Wang , Qing-Wen Tang , Yan-Qiu Zhang , Chao Zheng , Shao-Lin Xiong , Jia Ren , Bing Zhang
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