中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
First Detection of Ultrahigh Energy Emission from Gamma-Ray Binary LS I +61° 303

文献类型:期刊论文

作者Cao, Zhen1,2,3; Aharonian, F.3,4,5,6; Bai, Y. X.1,3; Bao, Y. W.7; Bastieri, D.8; Bi, X. J.1,2,3; Bi, Y. J.1,3; Bian, W.7; Bukevich, A. V.9; Cai, C. M.10
刊名Physical Review Letters
出版日期2026-05-08
卷号136期号:18
关键词Cosmic rays & astroparticles Gamma ray astronomy Binary stars
ISSN号0031-9007
DOI10.1103/7xhp-tff7
产权排序第26完成单位
文献子类Journal article (JA) -
英文摘要We report the first detection of gamma-ray emission up to ultrahigh-energy (UHE; >100 TeV) emission from the prototypical gamma-ray binary system LS I +61° 303 using data from the Large High Altitude Air Shower Observatory. It is detected with significances of 9.2σ in the Water Cherenkov Detector Array (WCDA, 1.4-30.5 TeV) and 6.2σ in the Kilometer Square Array (KM2A, 25-267 TeV); in KM2A alone we identify 16 photonlike events above 100 TeV against an estimated 5.1 background events, corresponding to a 3.8σ detection. These results provide compelling evidence of extreme particle acceleration in LS I +61° 303. Furthermore, we observe orbital modulation at 3.9σ confidence level, between 25 and 100 TeV, with a hint that the orbital modulation is energy dependent. These features can be understood in a composite scenario in which leptonic and hadronic processes jointly contribute. © 2026 American Physical Society.
学科主题天文学 ; 恒星与银河系 ; 星系与宇宙学
URL标识查看原文
资助项目N/A
语种英语
资助机构N/A
源URL[http://ir.ynao.ac.cn/handle/114a53/29246]  
专题星系类星体研究组
作者单位1.Key Laboratory of Particle Astrophysics and Experimental Physics Division and Computing Center, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing, 100049, China;
2.University of Chinese Academy of Sciences, Beijing, 100049, China;
3.TIANFU Cosmic Ray Research Center, Sichuan, Chengdu, China;
4.University of Science and Technology of China, Anhui, Hefei, 230026, China;
5.Yerevan State University, 1 Alek Manukyan Street, Yerevan, 0025, Armenia;
6.Max-Planck-Institut for Nuclear Physics, P.O. Box 103980, Heidelberg, 69029, Germany;
7.Tsung-Dao Lee Institute and School of Physics and Astronomy, Shanghai Jiao Tong University, Shanghai, 200240, China;
8.Center for Astrophysics, Guangzhou University, Guangdong, Guangzhou, 510006, China;
9.Institute for Nuclear Research of Russian Academy of Sciences, Moscow, 117312, Russia;
10.School of Physical Science and Technology and School of Information Science and Technology, Southwest Jiaotong University, Sichuan, Chengdu, 610031, China;
推荐引用方式
GB/T 7714
Cao, Zhen,Aharonian, F.,Bai, Y. X.,et al. First Detection of Ultrahigh Energy Emission from Gamma-Ray Binary LS I +61° 303[J]. Physical Review Letters,2026,136(18).
APA Cao, Zhen.,Aharonian, F..,Bai, Y. X..,Bao, Y. W..,Bastieri, D..,...&Qi, J. C..(2026).First Detection of Ultrahigh Energy Emission from Gamma-Ray Binary LS I +61° 303.Physical Review Letters,136(18).
MLA Cao, Zhen,et al."First Detection of Ultrahigh Energy Emission from Gamma-Ray Binary LS I +61° 303".Physical Review Letters 136.18(2026).

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