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A tera-electron volt afterglow from a narrow jet in an extremely bright gamma-ray burst
Cao, Zhen; Aharonian, F.6,7; An, Q.8,9; Axikegu10,11; Bai, L. X.12; Bai, Y. X.1,2,3,5; Bao, Y. W.13,40; Bastieri, D.14; Bi, X. J.1,2,3,4,5; Bi, Y. J.1,2,3,5; Cai, J. T.14; Cao, Q.15; Cao, W. Y.9; Cao, Zhe8,9; Chang, J.16,17; Chang, J. F.1,2,3,5,8; Chen, E. S.1,2,3,4,5; Chen, Liang18; Chen, Lin10,11; Chen, Long10,11; Chen, M. J.1,2,3,5; Chen, M. L.1,2,3,5,8; Chen, Q. H.10,11; Chen, S. H.1,2,3,4,5; Chen, S. Z.1,2,3,5; Chen, T. L.19; Chen, Y.13,40; Cheng, H. L.4,19,20; Cheng, N.1,2,3,5; Cheng, Y. D.1,2,3,5; Cui, S. W.15; Cui, X. H.20; Cui, Y. D.21,22,23; Dai, B. Z.24; Dai, H. L.1,2,3,5,8; Dai, Z. G.9; Danzengluobu19; della Volpe, D.25; Dong, X. Q.1,2,3,4,5; Duan, K. K.16,17; Fan, J. H.14; Fan, Y. Z.16,17; Fang, J.24; Fang, K.1,2,3,5; Feng, C. F.26; Feng, L.16,17; Feng, S. H.1,2,3,5; Feng, X. T.26; Feng, Y. L.19; Gao, B.1,2,3,5; Gao, C. D.26; Gao, L. Q.1,2,3,4,5; Gao, Q.19; Gao, W.1,2,3,5; Gao, W. K.1,2,3,4,5; Ge, M. M.24; Geng, L. S.1,2,3,5; Gong, G. H.27; Gou, Q. B.1,2,3,5; Gu, M. H.1,2,3,5,8; Guo, F. L.18; Guo, X. L.10,11; Guo, Y. Q.1,2,3,5; Guo, Y. Y.16,17; Han, Y. A.28; He, H. H.1,2,3,4,5; He, H. N.16,17; He, J. Y.16,17; He, X. B.21,22,23; He, Y.10,11; Heller, M.25; Hor, Y. K.21,22,23; Hou, B. W.1,2,3,4,5; Hou, C.1,2,3,5; Hou X(侯贤)29; Hu, H. B.1,2,3,4,5; Hu, Q.9,16,17; Hu, S. C.1,2,3,4,5; Huang, D. H.10,11; Huang, T. Q.1,2,3,5; Huang, W. J.21,22,23; Huang, X. T.26; Huang, X. Y.1,2,3,4,5,16,17; Huang, Y.1,2,3,4,5; Huang, Z. C.10,11; Ji, X. L.1,2,3,5,8; Jia, H. Y.10,11; Jia, K.26; Jiang, K.8,9; Jiang, X. W.1,2,3,5; Jiang, Z. J.24; Jin, M.10,11; Kang, M. M.12; Ke, T.1,2,3,5; Kuleshov, D.30; Kurinov, K.30,31; Li, B. B.15; Li, Cheng8,9; Li, Cong1,2,3,5; Li, D.1,2,3,4,5; Li, F.1,2,3,5,8; Li, H. B.1,2,3,5; Li, H. C.1,2,3,5; Li, H. Y.9,16,17; Li, J.9,16,17; Li, Jian9; Li, Jie1,2,3,5,8; Li, K.1,2,3,5; Li, W. L.26; Li, X. R.1,2,3,5; Li, Xin8,9; Li, Y. Z.1,2,3,4,5; Li, Zhe1,2,3,5; Li, Zhuo34; Liang, E. W.35; Liang, Y. F.35; Lin, S. J.21,22,23; Liu, B.9; Liu, C.1,2,3,5; Liu, D.26; Liu, H.10,11; Liu, H. D.28; Liu, J.1,2,3,5; Liu, J. L.1,2,3,5; Liu, J. S.21,22,23; Liu, J. Y.1,2,3,5; Liu, M. Y.19; Liu, R. Y.13,40; Liu, S. M.10,11; Liu, W.1,2,3,5; Liu, Y.14; Liu, Y. N.27; Long, W. J.10,11; Lu, R.24; Luo, Q.21,22,23; Lv, H. K.1,2,3,5; Ma, B. Q.34; Ma, L. L.1,2,3,5; Ma, X. H.1,2,3,5; Mao JR(毛基荣)29; Min, Z.1,2,3,5; Mitthumsiri, W.36; Nan, Y. C.1,2,3,5; Ou, Z. W.21,22,23; Pang, B. Y.10,11; Pattarakijwanich, P.36; Pei, Z. Y.14; Qi, M. Y.1,2,3,5; Qi, Y. Q.15; Qiao, B. Q.1,2,3,5; Qin, J. J.9; Ruffolo, D.36; Saiz, A.1,2,3,36; Shao, C. Y.21,22,23; Shao, L.15; Shchegolev, O.30,31; Sheng, X. D.1,2,3,5; Song, H. C.34; Stenkin, Y. V.30,31; Stepanov, V.30; Su, Y.16,17; Sun, Q. N.10,11; Sun, X. N.35; Sun, Z. B.37; Tam, P. H. T.21,22,23; Tang, Z. B.8,9; Tian, W. W.4,20; Wang, C.37; Wang, C. B.10,11; Wang, G. W.9; Wang, H. G.14; Wang, H. H.21,22,23; Wang JC(王建成)29; Wang, J. S.32,33; Wang, K.13,40; Wang, L. P.26; Wang, L. Y.1,2,3,5; Wang, P. H.10,11; Wang, R.26; Wang, W.13,21,22,23; Wang, X. G.35; Wang, X. Y.13,40; Wang, Y.10,11; Wang, Y. D.1,2,3,5; Wang, Y. J.1,2,3,5; Wang, Z. H.12; Wang, Z. X.24; Wang, Zhen32,33; Wang, Zheng1,2,3,5,8,13; Wei, D. M.16,17; Wei, J. J.16,17; Wei, Y. J.1,2,3,4,5; Wen, T.24; Wu, C. Y.1,2,3,5; Wu, H. R.1,2,3,5; Wu, S.1,2,3,5; Wu, X. F.16,17; Wu, Y. S.9; Xi, S. Q.1,2,3,5; Xia, J.9,16,17; Xia, J. J.10,11; Xiang, G. M.4,18; Xiao, D. X.15; Xiao, G.1,2,3,5; Xin, G. G.1,2,3,5; Xin, Y. L.10,11; Xing, Y.18; Xiong, Z.1,2,3,4,5; Xu, D. L.32,33; Xu, R. F.1,2,3,4,5; Xu, R. X.34; Xue, L.26; Yan, D. H.24; Yan, J. Z.16,17; Yan, T.1,2,3,5; Yang, C. W.12; Yang, F.15; Yang, F. F.1,2,3,5,8; Yang, H. W.21,22,23; Yang, J. Y.21,22,23; Yang, L. L.21,22,23; Yang, M. J.1,2,3,5; Yang, R. Z.9; Yang, S. B.24; Yao, Y. H.12; Yao, Z. G.1,2,3,5,16,17; Ye, Y. M.27; Yin, L. Q.1,2,3,5; Yin, N.26; You, X. H.1,2,3,5; You, Z. Y.1,2,3,4,5; Yu, Y. H.9; Yuan, Q.16,17; Yue, H.1,2,3,4,5; Zeng, H. D.16,17; Zeng, T. X.1,2,3,5,8; Zeng, W.24; Zeng, Z. K.1,2,3,4,5; Zha, M.1,2,3,5; Zhang, B.38,39; Zhang, B. B.13; Zhang, F.10,11; Zhang, H. M.13,40; Zhang, H. Y.1,2,3,5; Zhang, J. L.20; Zhang, L. X.14; Zhang, L.24; Zhang, P. F.24; Zhang, P. P.9,16,17; Zhang, R.9,16,17; Zhang, S. B.4,20; Zhang, S. R.15; Zhang, S. S.1,2,3,5; Zhang, X.13,40; Zhang, X. P.1,2,3,5; Zhang, Y. F.10,11; Zhang, Y.1,2,3,16,17; Zhang, Yong1,2,3,5; Zhao, B.10,11; Zhao, J.1,2,3,5; Zhao, L.8,9,16; Zhao, L. Z.15; Zhao, S. P.16,17,26; Zheng, F.37; Zheng, J. H.13,16,17,40; Zhou, B.1,2,3,5; Zhou, H.32,33; Zhou, J. N.18; Zhou, P.13; Zhou, R.12; Zhou, X. X.10,11; Zhu, C. G.26; Zhu, F. R.10,11; Zhu, H.20; Zhu, K. J.1,2,3,4,5,8; Zuo, X.1,2,3,5
发表期刊SCIENCE
2023-06-30
卷号380期号:6652
DOI10.1126/science.adg9328
产权排序第29完成单位
收录类别SCI
摘要Some gamma-ray bursts (GRBs) have a tera-electron volt (TeV) afterglow, but the early onset of this has not been observed. We report observations with the Large High Altitude Air Shower Observatory (LHAASO) of the bright GRB 221009A, which serendipitously occurred within the instrument's field of view. More than 64,000 photons >0.2 TeV were detected within the first 3000 seconds. The TeV flux began several minutes after the GRB trigger and then rose to a peak similar to 10 seconds later. This was followed by a decay phase, which became more rapid similar to 650 seconds after the peak. We interpret the emission using a model of a relativistic jet with half-opening angle of similar to 0.8 degrees. This is consistent with the core of a structured jet and could explain the high isotropic energy of this GRB.
资助项目National Key R&D program of China[2018YFA0404201]; National Key R&D program of China[2018YFA0404202]; National Key R&D program of China[2018YFA0404203]; National Key R&D program of China[2018YFA0404204]; NSFC[U1831208]; NSFC[11833003]; NSFC[12022502]; NSFC[12121003]; NSFC[U2031105]; NSFC[12005246]; NSFC[12173039]; NSFC[1221101008]; NSFC[12203022]; National SKA Program of China[2020SKA0120300]; Chinese Academy of Sciences[YSBR-061]; Department of Science and Technology of Sichuan Province[2021YFSY0030]; Natural Science Foundation of Jiangsu Province[BK20220757]; Chengdu Management Committee of Tianfu New Area; National Science and Technology Development Agency (NSTDA); National Research Council of Thailand (NRCT) under the High-Potential Research Team Grant Program[N42A650868]
项目资助者National Key R&D program of China[2018YFA0404201, 2018YFA0404202, 2018YFA0404203, 2018YFA0404204] ; NSFC[U1831208, 11833003, 12022502, 12121003, U2031105, 12005246, 12173039, 1221101008, 12203022] ; National SKA Program of China[2020SKA0120300] ; Chinese Academy of Sciences[YSBR-061] ; Department of Science and Technology of Sichuan Province[2021YFSY0030] ; Natural Science Foundation of Jiangsu Province[BK20220757] ; Chengdu Management Committee of Tianfu New Area ; National Science and Technology Development Agency (NSTDA) ; National Research Council of Thailand (NRCT) under the High-Potential Research Team Grant Program[N42A650868]
语种英语
学科领域天文学
文章类型Article
出版者AMER ASSOC ADVANCEMENT SCIENCE
出版地1200 NEW YORK AVE, NW, WASHINGTON, DC 20005 USA
ISSN0036-8075
URL查看原文
WOS记录号WOS:001161687500001
WOS研究方向Science & Technology - Other Topics
WOS类目Multidisciplinary Sciences
关键词[WOS]HIGH-ENERGY EMISSION ; SELF-COMPTON EMISSION ; LIGHT CURVES ; MODELS ; CONSTRAINTS ; SPECTRA ; SEARCH ; SHOCKS ; ONSET ; GRBS
引用统计
被引频次：59[WOS]   [WOS记录]     [WOS相关记录]
文献类型期刊论文
版本出版稿
条目标识符http://ir.ynao.ac.cn/handle/114a53/26440
专题星系类星体研究组
高能天体物理研究组
作者单位1.Chinese Acad Sci, Key Lab Particle Astrophys, Beijing 100049, Peoples R China;
2.Chinese Acad Sci, Expt Phys Div, Beijing 100049, Peoples R China;
3.Chinese Acad Sci, Inst High Energy Phys, Comp Ctr, Beijing 100049, Peoples R China;
4.Univ Chinese Acad Sci, Beijing 100049, Peoples R China;
5.Tianfu Cosm Ray Res Ctr, Chengdu 610000, Sichuan, Peoples R China;
6.Dublin Inst Adv Studies, 31 Fitzwilliam Pl, Dublin 2, Ireland;
7.Max Planck Inst Nucl Phys, POB 103980, D-69029 Heidelberg, Germany;
8.State Key Lab Particle Detect & Elect, Hefei, Peoples R China;
9.Univ Sci & Technol China, Hefei 230026, Anhui, Peoples R China;
10.Southwest Jiaotong Univ, Sch Phys Sci & Technol, Chengdu 610031, Sichuan, Peoples R China;
11.Southwest Jiaotong Univ, Sch Informat Sci & Technol, Chengdu 610031, Sichuan, Peoples R China;
12.Sichuan Univ, Coll Phys, Chengdu 610065, Sichuan, Peoples R China;
13.Nanjing Univ, Sch Astron & Space Sci, Nanjing 210023, Jiangsu, Peoples R China;
14.Guangzhou Univ, Ctr Astrophys, Guangzhou 510006, Guangdong, Peoples R China;
15.Hebei Normal Univ, Shijiazhuang 050024, Hebei, Peoples R China;
16.Chinese Acad Sci, Key Lab Dark Matter & Space Astron, Nanjing 210023, Jiangsu, Peoples R China;
17.Chinese Acad Sci, Key Lab Radio Astron, Purple Mt Observ, Nanjing 210023, Jiangsu, Peoples R China;
18.Chinese Acad Sci, Shanghai Astron Observ, Key Lab Res Galaxies & Cosmol, Shanghai 200030, Peoples R China;
19.Tibet Univ, Key Lab Cosm Rays, Minist Educ, Lhasa 850000, Tibet, Peoples R China;
20.Chinese Acad Sci, Natl Astron Observ, Beijing 100101, Peoples R China;
21.Sun Yat Sen Univ, Sch Phys & Astron Zhuhai, Zhuhai 519000, Guangdong, Peoples R China;
22.Sun Yat Sen Univ, Sch Phys Guangzhou, Guangzhou 510275, Guangdong, Peoples R China;
23.Sun Yat Sen Univ, Sino French Inst Nucl Engn & Technol Zhuhai, Zhuhai 519000, Guangdong, Peoples R China;
24.Yunnan Univ, Sch Phys & Astron, Kunming 650091, Yunnan, Peoples R China;
25.Univ Geneva, Fac Sci, Dept Phys Nucl & Corpusculaire, 24 Quai Ernest Ansermet, CH-1211 Geneva, Switzerland;
26.Shandong Univ, Inst Frontier & Interdisciplinary Sci, Qingdao 266237, Shandong, Peoples R China;
27.Tsinghua Univ, Dept Engn Phys, Beijing 100084, Peoples R China;
28.Zhengzhou Univ, Sch Phys & Microelect, Zhengzhou 450001, Henan, Peoples R China;
29.Chinese Acad Sci, Yunnan Observ, Kunming 650216, Yunnan, Peoples R China;
30.Russian Acad Sci, Inst Nucl Res, Moscow 117312, Russia;
31.Moscow Inst Phys & Technol, Moscow 141700, Russia;
32.Shanghai Jiao Tong Univ, Tsung Dao Lee Inst, Shanghai 200240, Peoples R China;
33.Shanghai Jiao Tong Univ, Sch Phys & Astron, Shanghai 200240, Peoples R China;
34.Peking Univ, Sch Phys, Beijing 100871, Peoples R China;
35.Guangxi Univ, Sch Phys Sci & Technol, Nanning 530004, Guangxi, Peoples R China;
36.Mahidol Univ, Fac Sci, Dept Phys, Bangkok 10400, Thailand;
37.Chinese Acad Sci, Natl Space Sci Ctr, Beijing 100190, Peoples R China;
38.Univ Nevada, Nevada Ctr Astrophys, Las Vegas, NV 89154 USA;
39.Univ Nevada, Dept Phys & Astron, Las Vegas, NV 89154 USA;
40.Nanjing Univ, Key Lab Modern Astron & Astrophys, Minist Educ, Nanjing 210023, Peoples R China
推荐引用方式
GB/T 7714		 Cao, Zhen,Aharonian, F.,An, Q.,et al. A tera-electron volt afterglow from a narrow jet in an extremely bright gamma-ray burst[J]. SCIENCE,2023,380(6652).
APA Cao, Zhen.,Aharonian, F..,An, Q..,Axikegu.,Bai, L. X..,...&Zuo, X..(2023).A tera-electron volt afterglow from a narrow jet in an extremely bright gamma-ray burst.SCIENCE,380(6652).
MLA Cao, Zhen,et al."A tera-electron volt afterglow from a narrow jet in an extremely bright gamma-ray burst".SCIENCE 380.6652(2023).
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