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A tera-electron volt afterglow from a narrow jet in an extremely bright gamma-ray burst.
Cao, Zhen; Aharonian, F; An, Q; Bai, L X; Bai, Y X; Bao, Y W; Bastieri, D; Bi, X J; Bi, Y J; Cai, J T; Cao, Q; Cao, W Y; Cao, Zhe; Chang, J; Chang, J F; 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; Cheng, H L; Cheng, N; Cheng, Y D; Cui, S W; Cui, X H; Cui, Y D; Dai, B Z; Dai, H L; Dai, Z G; Della Volpe, D; Dong, X Q; Duan, K K; Fan, J H; Fan, Y Z; Fang, J; Fang, K; Feng, C F; Feng, L; Feng, S H; Feng, X T; Feng, Y L; Gao, B; Gao, C D; Gao, L Q.
Afiliación
  • Cao Z; Key Laboratory of Particle Astrophysics & Experimental Physics Division & Computing Center, Institute of High Energy Physics, Chinese Academy of Sciences, 100049 Beijing, China.
  • Aharonian F; University of Chinese Academy of Sciences, 100049 Beijing, China.
  • An Q; Tianfu Cosmic Ray Research Center, 610000 Chengdu, Sichuan, China.
  • Axikegu; Dublin Institute for Advanced Studies, 31 Fitzwilliam Place, 2 Dublin, Ireland.
  • Bai LX; Max-Planck-Institute for Nuclear Physics, P.O. Box 103980, 69029 Heidelberg, Germany.
  • Bai YX; State Key Laboratory of Particle Detection and Electronics, China.
  • Bao YW; University of Science and Technology of China, 230026 Hefei, Anhui, China.
  • Bastieri D; School of Physical Science and Technology & School of Information Science and Technology, Southwest Jiaotong University, 610031 Chengdu, Sichuan, China.
  • Bi XJ; College of Physics, Sichuan University, 610065 Chengdu, Sichuan, China.
  • Bi YJ; Key Laboratory of Particle Astrophysics & Experimental Physics Division & Computing Center, Institute of High Energy Physics, Chinese Academy of Sciences, 100049 Beijing, China.
  • Cai JT; Tianfu Cosmic Ray Research Center, 610000 Chengdu, Sichuan, China.
  • Cao Q; School of Astronomy and Space Science, Nanjing University, 210023 Nanjing, Jiangsu, China.
  • Cao WY; Key Laboratory of Modern Astronomy and Astrophysics (Nanjing University), Ministry of Education, Nanjing 210023, China.
  • Cao Z; Center for Astrophysics, Guangzhou University, 510006 Guangzhou, Guangdong, China.
  • Chang J; Key Laboratory of Particle Astrophysics & Experimental Physics Division & Computing Center, Institute of High Energy Physics, Chinese Academy of Sciences, 100049 Beijing, China.
  • Chang JF; University of Chinese Academy of Sciences, 100049 Beijing, China.
  • Chen ES; Tianfu Cosmic Ray Research Center, 610000 Chengdu, Sichuan, China.
  • Chen L; Key Laboratory of Particle Astrophysics & Experimental Physics Division & Computing Center, Institute of High Energy Physics, Chinese Academy of Sciences, 100049 Beijing, China.
  • Chen L; Tianfu Cosmic Ray Research Center, 610000 Chengdu, Sichuan, China.
  • Chen L; Center for Astrophysics, Guangzhou University, 510006 Guangzhou, Guangdong, China.
  • Chen MJ; Hebei Normal University, 050024 Shijiazhuang, Hebei, China.
  • Chen ML; University of Science and Technology of China, 230026 Hefei, Anhui, China.
  • Chen QH; State Key Laboratory of Particle Detection and Electronics, China.
  • Chen SH; University of Science and Technology of China, 230026 Hefei, Anhui, China.
  • Chen SZ; Key Laboratory of Dark Matter and Space Astronomy & Key Laboratory of Radio Astronomy, Purple Mountain Observatory, Chinese Academy of Sciences, 210023 Nanjing, Jiangsu, China.
  • Chen TL; Key Laboratory of Particle Astrophysics & Experimental Physics Division & Computing Center, Institute of High Energy Physics, Chinese Academy of Sciences, 100049 Beijing, China.
  • Chen Y; Tianfu Cosmic Ray Research Center, 610000 Chengdu, Sichuan, China.
  • Cheng HL; State Key Laboratory of Particle Detection and Electronics, China.
  • Cheng N; Key Laboratory of Particle Astrophysics & Experimental Physics Division & Computing Center, Institute of High Energy Physics, Chinese Academy of Sciences, 100049 Beijing, China.
  • Cheng YD; University of Chinese Academy of Sciences, 100049 Beijing, China.
  • Cui SW; Tianfu Cosmic Ray Research Center, 610000 Chengdu, Sichuan, China.
  • Cui XH; Key Laboratory for Research in Galaxies and Cosmology, Shanghai Astronomical Observatory, Chinese Academy of Sciences, 200030 Shanghai, China.
  • Cui YD; School of Physical Science and Technology & School of Information Science and Technology, Southwest Jiaotong University, 610031 Chengdu, Sichuan, China.
  • Dai BZ; School of Physical Science and Technology & School of Information Science and Technology, Southwest Jiaotong University, 610031 Chengdu, Sichuan, China.
  • Dai HL; Key Laboratory of Particle Astrophysics & Experimental Physics Division & Computing Center, Institute of High Energy Physics, Chinese Academy of Sciences, 100049 Beijing, China.
  • Dai ZG; Tianfu Cosmic Ray Research Center, 610000 Chengdu, Sichuan, China.
  • Danzengluobu; Key Laboratory of Particle Astrophysics & Experimental Physics Division & Computing Center, Institute of High Energy Physics, Chinese Academy of Sciences, 100049 Beijing, China.
  • Della Volpe D; Tianfu Cosmic Ray Research Center, 610000 Chengdu, Sichuan, China.
  • Dong XQ; State Key Laboratory of Particle Detection and Electronics, China.
  • Duan KK; School of Physical Science and Technology & School of Information Science and Technology, Southwest Jiaotong University, 610031 Chengdu, Sichuan, China.
  • Fan JH; Key Laboratory of Particle Astrophysics & Experimental Physics Division & Computing Center, Institute of High Energy Physics, Chinese Academy of Sciences, 100049 Beijing, China.
  • Fan YZ; University of Chinese Academy of Sciences, 100049 Beijing, China.
  • Fang J; Tianfu Cosmic Ray Research Center, 610000 Chengdu, Sichuan, China.
  • Fang K; Key Laboratory of Particle Astrophysics & Experimental Physics Division & Computing Center, Institute of High Energy Physics, Chinese Academy of Sciences, 100049 Beijing, China.
  • Feng CF; Tianfu Cosmic Ray Research Center, 610000 Chengdu, Sichuan, China.
  • Feng L; Key Laboratory of Cosmic Rays (Tibet University), Ministry of Education, 850000 Lhasa, Tibet, China.
  • Feng SH; School of Astronomy and Space Science, Nanjing University, 210023 Nanjing, Jiangsu, China.
  • Feng XT; Key Laboratory of Modern Astronomy and Astrophysics (Nanjing University), Ministry of Education, Nanjing 210023, China.
  • Feng YL; University of Chinese Academy of Sciences, 100049 Beijing, China.
  • Gao B; Key Laboratory of Cosmic Rays (Tibet University), Ministry of Education, 850000 Lhasa, Tibet, China.
Science ; 380(6652): 1390-1396, 2023 Jun 30.
Article en En | MEDLINE | ID: mdl-37289911
ABSTRACT
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 ~10 seconds later. This was followed by a decay phase, which became more rapid ~650 seconds after the peak. We interpret the emission using a model of a relativistic jet with half-opening angle of ~0.8°. This is consistent with the core of a structured jet and could explain the high isotropic energy of this GRB.
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Texto completo: 1 Colección: 01-internacional Banco de datos: MEDLINE Idioma: En Revista: Science Año: 2023 Tipo del documento: Article País de afiliación: China
Texto completo
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XML
PubMed Links
Buscar en Google

Texto completo: 1 Colección: 01-internacional Banco de datos: MEDLINE Idioma: En Revista: Science Año: 2023 Tipo del documento: Article País de afiliación: China