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We present broadband (gamma-ray, X-ray, near-infrared, optical, and radio) observations of the gamma-ray burst (GRB) 090709A and its afterglow in an effort to ascertain the origin of this high-energy transient. Previous analyses suggested…

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…

Gamma-ray bursts (GRBs) are powerful probes of early stars and galaxies, during and potentially even before the era of reionization. Although the number of GRBs identified at z>6 remains small, they provide a unique window on typical…

We report on the detection of a very rapid TeV gamma-ray flare from BL Lacertae on 2011 June 28 with the Very Energetic Radiation Imaging Telescope Array System (VERITAS). The flaring activity was observed during a 34.6-minute exposure,…

The high energy GeV emission of gamma-ray bursts (GRBs), detected by \emph{Fermi}/LAT, has a significantly different morphology compared to the lower energy MeV emission, detected by \emph{Fermi}/GBM. Though the late time GeV emission is…

High Energy Astrophysical Phenomena · Physics 2015-06-16 Rupal Basak , A. R. Rao

The Gamma Ray Burst GRB920229 has four extreme and unprecedented properties; a rise in brightness with an e-folding time scale of $220 \pm 30 \mu s$, a fall in brightness with an e-folding time scale of $400 \pm 100 \mu s$, a large change…

Astrophysics · Physics 2009-10-31 Bradley E. Schaefer , Katharine C. Walker

As the brightest gamma-ray burst ever observed, GRB 221009A provided a precious opportunity to explore spectral line features. In this paper, we performed a comprehensive spectroscopy analysis of GRB 221009A jointly with GECAM-C and…

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 130427A was extremely bright as a result of occurring at low redshift whilst the energetics were more typical of high-redshift gamma-ray bursts (GRBs). We collected well-sampled light curves at 1.4 and 4.8 GHz of GRB 130427A with the…

GRB160203A is a high redshift long gamma-ray burst presenting a collection of unusual features in the afterglow light curve. We study its optical and X-ray data. We find this event to occur within a constant density medium during the first…

High Energy Astrophysical Phenomena · Physics 2021-04-14 H. Crisp , B. Gendre , E. J. Howell , D. Coward

GRB 221009A is the brightest gamma-ray burst (GRB) observed to date. Extensive observations of its afterglow emission across the electromagnetic spectrum were performed, providing the first strong evidence of a jet with a nontrivial angular…

High Energy Astrophysical Phenomena · Physics 2026-03-11 LST Collaboration , K. Abe , S. Abe , A. Abhishek , F. Acero , A. Aguasca-Cabot , I. Agudo , C. Alispach , D. Ambrosino , F. Ambrosino , L. A. Antonelli , C. Aramo , A. Arbet-Engels , C. Arcaro , T. T. H. Arnesen , K. Asano , P. Aubert , A. Baktash , M. Balbo , A. Bamba , A. Baquero Larriva , U. Barres de Almeida , J. A. Barrio , L. Barrios Jiménez , I. Batkovic , J. Baxter , J. Becerra González , E. Bernardini , J. Bernete , A. Berti , I. Bezshyiko , C. Bigongiari , E. Bissaldi , O. Blanch , G. Bonnoli , P. Bordas , G. Borkowski , G. Brunelli , A. Bulgarelli , M. Bunse , I. Burelli , L. Burmistrov , M. Cardillo , S. Caroff , A. Carosi , R. Carraro , M. S. Carrasco , F. Cassol , D. Cerasole , G. Ceribella , A. Cerviño Cortínez , Y. Chai , K. Cheng , A. Chiavassa , M. Chikawa , G. Chon , L. Chytka , G. M. Cicciari , A. Cifuentes , J. L. Contreras , J. Cortina , H. Costantini , M. Dalchenko , P. Da Vela , F. Dazzi , A. De Angelis , M. de Bony de Lavergne , R. Del Burgo , C. Delgado , J. Delgado Mengual , M. Dellaiera , D. della Volpe , B. De Lotto , L. Del Peral , R. de Menezes , G. De Palma , C. Díaz , A. Di Piano , F. Di Pierro , R. Di Tria , L. Di Venere , R. M. Dominik , D. Dominis Prester , A. Donini , D. Dorner , M. Doro , L. Eisenberger , D. Elsässer , G. Emery , J. Escudero , V. Fallah Ramazani , F. Ferrarotto , A. Fiasson , L. Foffano , F. Frías García-Lago , S. Fröse , Y. Fukazawa , S. Gallozzi , R. Garcia López , S. Garcia Soto , C. Gasbarra , D. Gasparrini , D. Geyer , J. Giesbrecht Paiva , N. Giglietto , F. Giordano , N. Godinovic , T. Gradetzke , R. Grau , D. Green , J. Green , S. Gunji , P. Günther , J. Hackfeld , D. Hadasch , A. Hahn , M. Hashizume , T. Hassan , K. Hayashi , L. Heckmann , M. Heller , J. Herrera Llorente , K. Hirotani , D. Hoffmann , D. Horns , J. Houles , M. Hrabovsky , D. Hrupec , D. Hui , M. Iarlori , R. Imazawa , T. Inada , Y. Inome , S. Inoue , K. Ioka , M. Iori , T. Itokawa , A. Iuliano , J. Jahanvi , I. Jimenez Martinez , J. Jimenez Quiles , I. Jorge Rodrigo , J. Jurysek , M. Kagaya , O. Kalashev , V. Karas , H. Katagiri , D. Kerszberg , T. Kiyomot , Y. Kobayashi , K. Kohri , A. Kong , P. Kornecki , H. Kubo , J. Kushida , B. Lacave , M. Lainez , G. Lamanna , A. Lamastra , L. Lemoigne , M. Linhoff , S. Lombardi , F. Longo , R. López-Coto , M. López-Moya , A. López-Oramas , S. Loporchio , A. Lorini , J. Lozano Bahilo , F. Lucarelli , H. Luciani , P. L. Luque-Escamilla , P. Majumdar , M. Makariev , M. Mallamaci , D. Mandat , M. Manganaro , D. K. Maniadakis , G. Manicò , K. Mannheim , S. Marchesi , F. Marini , M. Mariotti , P. Marquez , G. Marsella , J. Martí , O. Martinez , G. Martínez , M. Martínez , A. Mas-Aguilar , M. Massa , G. Maurin , D. Mazin , J. Méndez-Gallego , S. Menon , E. Mestre Guillen , D. Miceli , T. Miener , J. M. Miranda , R. Mirzoyan , M. Mizote , T. Mizuno , M. Molero Gonzalez , E. Molina , T. Montaruli , A. Moralejo , D. Morcuende , A. Moreno Ramos , A. Morselli , V. Moya , H. Muraishi , S. Nagataki , T. Nakamori , A. Neronov , D. Nieto Castaño , M. Nievas Rosillo , L. Nikolic , K. Nishijima , K. Noda , D. Nosek , V. Novotny , S. Nozaki , M. Ohishi , Y. Ohtani , T. Oka , A. Okumura , R. Orito , L. Orsini , J. Otero-Santos , P. Ottanelli , M. Palatiello , G. Panebianco , D. Paneque , F. R. Pantaleo , R. Paoletti , J. M. Paredes , M. Pech , M. Pecimotika , M. Peresano , F. Pfeifle , E. Pietropaolo , M. Pihet , G. Pirola , C. Plard , F. Podobnik , M. Polo , E. Prandini , M. Prouza , S. Rainò , R. Rando , W. Rhode , M. Ribó , V. Rizi , G. Rodriguez Fernandez , M. D. Rodríguez Frías , P. Romano , A. Roy , A. Ruina , E. Ruiz-Velasco , T. Saito , S. Sakurai , D. A. Sanchez , H. Sano , T. Šarić , Y. Sato , F. G. Saturni , V. Savchenko , F. Schiavone , B. Schleicher , F. Schmuckermaier , J. L. Schubert , F. Schussler , T. Schweizer , M. Seglar Arroyo , T. Siegert , G. Silvestri , A. Simongini , J. Sitarek , V. Sliusar , A. Stamerra , J. Strišković , M. Strzys , Y. Suda , A. Sunny , H. Tajima , M. Takahashi , J. Takata , R. Takeishi , P. H. T. Tam , S. J. Tanaka , D. Tateishi , T. Tavernier , P. Temnikov , Y. Terada , K. Terauchi , T. Terzic , M. Teshima , M. Tluczykont , F. Tokanai , T. Tomura , D. F. Torres , F. Tramonti , P. Travnicek , G. Tripodo , A. Tutone , M. Vacula , J. van Scherpenberg , M. Vázquez Acosta , S. Ventura , S. Vercellone , G. Verna , I. Viale , A. Vigliano , C. F. Vigorito , E. Visentin , V. Vitale , V. Voitsekhovskyi , G. Voutsinas , I. Vovk , T. Vuillaume , R. Walter , L. Wan , M. Will , J. Wójtowicz , T. Yamamoto , R. Yamazaki , Y. Yao , P. K. H. Yeung , T. Yoshida , T. Yoshikoshi , W. Zhang

Gamma-ray bursts (GRBs) are the most powerful explosions in the universe and probe physics under extreme conditions. GRBs divide into two classes, of short and long duration, thought to originate from different types of progenitor systems.…

High Energy Astrophysical Phenomena · Physics 2014-11-20 LAT Collaboration

The spectral evolution characteristics of the prompt emission in gamma-ray bursts (GRBs) have been extensively studied, but detailed investigations of spectral evolution in a GRB flare remain lacking. In this work, we present the first…

The most energetic gamma-ray bursts (GRBs) are remarkable sources releasing huge amounts of energy on short timescales. Their prompt emission, which usually lasts few seconds, is so bright that it is visible across the whole observable…

High Energy Astrophysical Phenomena · Physics 2017-12-07 J-L. Atteia , V. Heussaff , J. -P. Dezalay , A. Klotz , D. Turpin , A. E. Tsvetkova , D. D. Frederiks , Y. Zolnierowski , F. Daigne , R. Mochkovitch

Here we report on the detailed analysis of the gamma-ray light curve of a luminous blazar PKS1510-089 observed in the GeV range with the Large Area Telescope (LAT) onboard the Fermi satellite during the period 2011 September -- December. By…

High Energy Astrophysical Phenomena · Physics 2015-06-12 S. Saito , L. Stawarz , Y. T. Tanaka , T. Takahashi , G. Madejski , F. D'Ammando

We report on the observation of the bright, long gamma-ray burst, GRB 090926A, by the Gamma-ray Burst Monitor (GBM) and Large Area Telescope (LAT) instruments on board the \Fermi\ Gamma-ray Space Telescope. GRB 090926A shares several…

High Energy Astrophysical Phenomena · Physics 2015-03-17 Fermi-LAT , Fermi-GBM collaborations

We present a discovery and observation of an extraordinarily bright prompt optical emission of the GRB 060117 obtained by a wide-field camera atop the robotic telescope FRAM of the Pierre Auger Observatory from 2 to 10 minutes after the…

GRB 130925A was an unusual GRB, consisting of 3 distinct episodes of high-energy emission spanning $\sim$20 ks, making it a member of the proposed category of `ultra-long' bursts. It was also unusual in that its late-time X-ray emission…

Violent multi-wavelength variabilities are observed in gamma-ray-selected blazars. We present an analysis of long-term light curves for eight bright blazars to explore the co-variation pattern in the gamma-ray and radio bands. We extract…

High Energy Astrophysical Phenomena · Physics 2020-05-27 Hai-Ming Zhang , Zhen-Jie Wang , Jin Zhang , Ting-Feng Yi , Liang Chen , Rui-Jing Lu , En-Wei Liang

We report the discovery of high-energy \gamma-ray emission from the Broad Line Radio Galaxy (BLRG) Pictor A with a significance of ~5.8\sigma (TS=33.4), based on three years of observations with the Fermi Large Area Telescope (LAT)…

High Energy Astrophysical Phenomena · Physics 2015-06-03 Anthony M. Brown , Jenni Adams