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Measurement of very-high-energy diffuse gamma-ray emission from |b|<5◦ of the Galactic plane with LHAASO-WCDA
Li, Huicai1,4; Zhang, Peipei1,13; Hu, Shicong1,4; Zha, Min1,4; Guo, Yiqing1,4; Yuan, Qiang13; Yao, Zhiguo1,4; Cao, Zhen2,3,4,18; Aharonian, F.5,6; An, Q.7,8; Axikegu9; Bai, Y. X.2,4; Bao, Y. W.10; Bastieri, D.11; Bi, X. J.2,3,4; Bi, Y. J.2,4; Cai, J. T.11; Cao, Q.12; Cao, W. Y.8; Cao, Zhe7,8; Chang, J.13; Chang, J. F.2,4,7; Chen, A. M.14; Chen, E. S.2,3,4; Chen, Liang15; Chen, Lin9; Chen, Long9; Chen, M. J.2,4; Chen, M. L.2,4,7; Chen, Q. H.9; Chen, S. H.2,3,4,18; Chen, S. Z.2,4; Chen, T. L.16; Chen, Y.10; Cheng, N.2,4; Cheng, Y. D.2,4; Cui, M. Y.13; Cui, S. W.12; Cui, X. H.17; Cui, Y. D.18; Dai, B. Z.19; Dai, H. L.2,4,7; Dai, Z. G.8; Danzengluobu16; della Volpe, D.20; Dong, X. Q.2,3,4; Duan, K. K.13; Fan, J. H.11; Fan, Y. Z.13; Fang, J.19; Fang, K.2,4; Feng, C. F.21; Feng, L.13; Feng, S. H.2,4; Feng, X. T.21; Feng, Y. L.16; Gabici, S.22; Gao, B.2,4; Gao, C. D.21; Gao, L. Q.2,3,4; Gao, Q.16; Gao, W.2,4; Gao, W. K.2,3,4; Ge, M. M.19; Geng, L. S.2,4; Giacinti, G.14; Gong, G. H.23; Gou, Q. B.2,4; Gu, M. H.2,4,7; Guo, F. L.15; Guo, X. L.9; Guo, Y. Q.2,4; Guo, Y. Y.13; Han, Y. A.24; He, H. H.2,3,4; He, H. N.13; He, J. Y.13; He, X. B.18; He, Y.9; Heller, M.20; Hor, Y. K.18; Hou, B. W.2,3,4; Hou, C.2,4; Hou X(侯贤)25; Hu, H. B.2,3,4; Hu, Q.8,13; Hu, S. C.2,3,4; Huang, D. H.9; Huang, T. Q.2,4; Huang, W. J.18; Huang, X. T.21; Huang, X. Y.13; Huang, Y.2,3,4; Huang, Z. C.9; Ji, X. L.2,4,7; Jia, H. Y.9; Jia, K.21; Jiang, K.7,8; Jiang, X. W.2,4; Jiang, Z. J.19; Jin, M.9; Kang, M. M.26; Ke, T.2,4; Kuleshov, D.27; Kurinov, K.27; Li, B. B.12; Li, Cheng7,8; Li, Cong2,4; Li, D.2,3,4; Li, F.2,4,7; Li, H. B.2,4; Li, H. C.2,4; Li, H. Y.8,13; Li, J.8,13; Li, Jian8; Li, Jie2,4,7; Li, K.2,4; Li, W. L.21; Li, W. L.14; Li, X. R.2,4; Li, Xin7,8; Li, Y. Z.2,3,4; Li, Zhe2,4; Li, Zhuo28; Liang, E. W.29; Liang, Y. F.29; Lin, S. J.18; Liu, B.8; Liu, C.2,4; Liu, D.21; Liu, H.9; Liu, H. D.24; Liu, J.2,4; Liu, J. L.2,4; Liu, J. Y.2,4; Liu, M. Y.16; Liu, R. Y.10; Liu, S. M.9; Liu, W.2,4; Liu, Y.11; Liu, Y. N.23; Lu, R.19; Luo, Q.18; Lv, H. K.2,4; Ma, B. Q.28; Ma, L. L.2,4; Ma, X. H.2,4; Mao JR(毛基荣)25; Min, Z.2,4; Mitthumsiri, W.30; Mu, H. J.24; Nan, Y. C.2,4; Neronov, A.22; Ou, Z. W.18; Pang, B. Y.9; Pattarakijwanich, P.30; Pei, Z. Y.11; Qi, M. Y.2,4; Qi, Y. Q.12; Qiao, B. Q.2,4; Qin, J. J.8; Ruffolo, D.30; Sáiz, A.30; Semikoz, D.22; Shao, C. Y.18; Shao, L.12; Shchegolev, O.27,31; Sheng, X. D.2,4; Shu, F. W.32; Song, H. C.28; Stenkin, Yu. V.27,31; Stepanov, V.27; Su, Y.13
会议录名称Proceedings of Science
2024-09-27
卷号444
DOI10.22323/1.444.0672
产权排序第25完成单位
收录类别EI
会议名称38th International Cosmic Ray Conference, ICRC 2023
会议日期2023-07-26
会议地点Nagoya, Japan
会议赞助商et al.; Institute for Cosmic Ray Research (ICRR) Univeristy of Tokyo; International Union of Pure and Applied Physics (IUPAP); JPS; Nagoya Convention and Visitors Bureau; Nagoya University
摘要Galactic diffuse gamma ray emission (GDE) is introduced by the galactic cosmic rays (CR) interacting with the interstellar medium (ISM) and radiation fields (ISRF). The GDE is a very important probe of CR propagation and interaction. Different from the measurements of CR particles in the local vicinity, the GDE enables a direct measurement of CR distribution in the Milky Way, and can thus provide much more important information of the production and propagation of CRs. LHAASO-WCDA, with an large area of 78000 m2, has an excellent ability to study VHE gamma-ray astronomy and GDE. In this proceeding, method of background estimation and some techniques to reduce the contaminant of resolved gamma-ray sources are briefly introduced. At last, diffuse emissions from the inner (15◦ ◦, |b| ◦) and outer (125◦ ◦, |b| ◦) Galactic plane are detected with 27.9σ and 11.9σ significance, respectively. © Copyright owned by the author(s) under the terms of the Creative Commons.
资助项目N/A
项目资助者N/A
语种英语
学科领域天文学 ; 天体物理学 ; 高能天体物理学 ; 星系与宇宙学
文章类型Conference article (CA)
URL查看原文
EI入藏号20245117555915
EI主题词Gamma rays
EI分类号1301.2.1 - 1301.2.2 - 1302.1 - 1303.1 - 941.5 - 941.9 - 942.1.7
引用统计
文献类型会议论文
条目标识符http://ir.ynao.ac.cn/handle/114a53/27920
专题星系类星体研究组
作者单位1.Institute of High Energy Physics, Chinese Academy of Sciences, Beijing, 100049, China;
2.Key Laboratory of Particle Astrophyics & Experimental Physics Division & Computing Center, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing, 100049, China;
3.University of Chinese Academy of Sciences, Beijing, 100049, China;
4.TIANFU Cosmic Ray Research Center, Sichuan, Chengdu, China;
5.Dublin Institute for Advanced Studies, 31 Fitzwilliam Place, 2, Dublin, Ireland;
6.Max-Planck-Institut for Nuclear Physics, P.O. Box 103980, Heidelberg, 69029, Germany;
7.State Key Laboratory of Particle Detection and Electronics, China;
8.University of Science and Technology of China, Anhui, Hefei, 230026, China;
9.School of Physical Science and Technology, School of Information Science and Technology, Southwest Jiaotong University, Sichuan, Chengdu, 610031, China;
10.School of Astronomy and Space Science, Nanjing University, Jiangsu, Nanjing, 210023, China;
11.Center for Astrophysics, Guangzhou University, Guangdong, Guangzhou, 510006, China;
12.Hebei Normal University, Hebei, Shijiazhuang, 050024, China;
13.Key Laboratory of Dark Matter and Space Astronomy, Key Laboratory of Radio Astronomy, Purple Mountain Observatory, Chinese Academy of Sciences, Jiangsu, Nanjing, 210023, China;
14.Tsung-Dao Lee Institute, School of Physics and Astronomy, Shanghai Jiao Tong University, Shanghai, 200240, China;
15.Key Laboratory for Research in Galaxies and Cosmology, Shanghai Astronomical Observatory, Chinese Academy of Sciences, Shanghai, 200030, China;
16.Key Laboratory of Cosmic Rays (Tibet University), Ministry of Education, Tibet, Lhasa, 850000, China;
17.National Astronomical Observatories, Chinese Academy of Sciences, Beijing, 100101, China;
18.School of Physics and Astronomy (Zhuhai), School of Physics (Guangzhou), Sino-French Institute of Nuclear Engineering and Technology (Zhuhai), Sun Yat-sen University, Guangdong, Guangzhou, 510275, China;
19.School of Physics and Astronomy, Yunnan University, Yunnan, Kunming, 650091, China;
20.Département de Physique Nucléaire et Corpusculaire, Faculté de Sciences, Université de Genève, 24 Quai Ernest Ansermet, Geneva, 1211, Switzerland;
21.Institute of Frontier and Interdisciplinary Science, Shandong University, Shandong, Qingdao, 266237, China;
22.APC, Université Paris Cité, CNRS, IN2P3, CEA, IRFU, Observatoire de Paris, Paris, 119 75205, France;
23.Department of Engineering Physics, Tsinghua University, Beijing, 100084, China;
24.School of Physics and Microelectronics, Zhengzhou University, Henan, Zhengzhou, 450001, China;
25.Yunnan Observatories, Chinese Academy of Sciences, Yunnan, Kunming, 650216, China;
26.College of Physics, Sichuan University, Sichuan, Chengdu, 610065, China;
27.Institute for Nuclear Research of Russian Academy of Sciences, Moscow, 117312, Russia;
28.School of Physics, Peking University, Beijing, 100871, China;
29.School of Physical Science and Technology, Guangxi University, Guangxi, Nanning, 530004, China;
30.Department of Physics, Faculty of Science, Mahidol University, Bangkok, 10400, Thailand;
31.Moscow Institute of Physics and Technology, Moscow, 141700, Russia;
32.Center for Relativistic Astrophysics and High Energy Physics, School of Physics and Materials Science, Institute of Space Science and Technology, Nanchang University, Jiangxi, Nanchang, 330031, China;
33.National Space Science Center, Chinese Academy of Sciences, Beijing, 100190, China
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Li, Huicai,Zhang, Peipei,Hu, Shicong,et al. Measurement of very-high-energy diffuse gamma-ray emission from |b|<5◦ of the Galactic plane with LHAASO-WCDA[C],2024.
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