Measurement of ultra-high-energy diffuse gamma-ray emission of the Galactic plane from 10 TeV to 1 PeV with LHAASO-KM2A

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【作者】Cao, Zhen， Aharonian, F.， An, Q.， Axikegu， 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, A.M.， Chen, E.S.， Chen, Liang， Chen, Lin， Chen, Long， Chen, M.J.， M.L., Chen， Q.H., Chen， S.H., Chen， S.Z., Chen， T.L., Chen， Y., Chen， N., Cheng， Y.D., Cheng， M.Y., Cui， S.W., Cui， X.H., Cui， Y.D., Cui， B.Z., Dai， H.L., Dai， Z.G., Dai， 15， D., della Volpe， X.Q., Dong， K.K., Duan， J.H., Fan， Y.Z., Fan， J., Fang， K., Fang， C.F., Feng， L., Feng， S.H., Feng， X.T., Feng， Y.L., Feng， S., Gabici， B., Gao， C.D., Gao， L.Q., Gao， Q., Gao， W., Gao， W.K., Gao， M.M., Ge， L.S., Geng， G., Giacinti， G.H., Gong， Q.B., Gou， M.H., Gu， F.L., Guo， X.L., Guo， Y.Q., Guo， Y.Y., Guo， Y.A., Han， H.H., He， H.N., He， J.Y., He， X.B., He， Y., He， M., Heller， Y.K., Hor， B.W., Hou， C., Hou， X., Hou， H.B., Hu， Q., Hu， S.C., Hu， D.H., Huang， T.Q., Huang， W.J., Huang， X.T., Huang， X.Y., Huang， Y., Huang， Z.C., Huang， X.L., Ji， H.Y., Jia， K., Jia， K., Jiang， X.W., Jiang， Z.J., Jiang， M., Jin， M.M., Kang， T., Ke， D., Kuleshov， K., Kurinov， B.B., Li， C., Li， C., Li， D., Li， F., Li， H.B., Li， H.C., Li， H.Y., Li， J., Li， J., Li， J., Li， K., Li， W.L., Li， W.L., Li， X.R., Li， X., Li， Y.Z., Li， Z., Li， Z., Li， E.W., Liang， Y.F., Liang， S.J., Lin， B., Liu， C., Liu， D., Liu， H., Liu， H.D., Liu， J., Liu， J.L., Liu， J.Y., Liu， M.Y., Liu， R.Y., Liu， S.M., Liu， W., Liu， Y., Liu， Y.N., Liu， R., Lu， Q., Luo， H.K., Lv， B.Q., Ma， L.L., Ma， X.H., Ma， J.R., Mao， Z., Min， W., Mitthumsiri， H.J., Mu， Y.C., Nan， A., Neronov， Z.W., Ou， B.Y., Pang， P., Pattarakijwanich， Z.Y., Pei， M.Y., Qi， Y.Q., Qi， B.Q., Qiao， J.J., Qin， D., Ruffolo， A., Sáiz， D., Semikoz， C.Y., Shao， L., Shao， O., Shchegolev， X.D., Sheng， F.W., Shu， H.C., Song， Y.V., Stenkin， V., Stepanov， Y., Su， Q.N., Sun， X.N., Sun， Z.B., Sun， P.H.T., Tam
【作者单位】¹Key Laboratory of Particle Astrophyics & Experimental Physics Division & Computing Center, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing; 100049, China;²University of Chinese Academy of Sciences, Beijing; 100049, China;³Tianfu Cosmic Ray Research Center, Sichuan, Chengdu; 610000, China;⁴Dublin Institute for Advanced Studies, 31 Fitzwilliam Place, Dublin 2, Ireland;⁵Max-Planck-Institut for Nuclear Physics, P.O. Box 103980, Heidelberg; 69029, Germany;⁶State Key Laboratory of Particle Detection and Electronics, China;⁷University of Science and Technology of China, Anhui, Hefei; 230026, China;⁸School of Physical Science and Technology, School of Information Science and Technology, Southwest Jiaotong University, Sichuan, Chengdu; 610031, China;⁹School of Astronomy and Space Science, Nanjing University, Jiangsu, Nanjing; 210023, China;¹⁰Center for Astrophysics, Guangzhou University, Guangdong, Guangzhou; 510006, China;¹¹Hebei Normal University, Hebei, Shijiazhuang; 050024, China;¹²Key Laboratory of Dark Matter and Space Astronomy, Key Laboratory of Radio Astronomy, Purple Mountain Observatory, Chinese Academy of Sciences, Jiangsu, Nanjing; 210023, China;¹³Tsung-Dao Lee Institute, School of Physics and Astronomy, Shanghai Jiao Tong University, Shanghai; 200240, China;¹⁴Key Laboratory for Research in Galaxies and Cosmology, Shanghai Astronomical Observatory, Chinese Academy of Sciences, Shanghai; 200030, China;¹⁵Key Laboratory of Cosmic Rays (Tibet University, Ministry of Education, Tibet, Lhasa; 850000, China;¹⁶National Astronomical Observatories, Chinese Academy of Sciences, Beijing; 100101, China;¹⁷School 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;¹⁸School of Physics and Astronomy, Yunnan University, Yunnan, Kunming; 650091, China;¹⁹Département de Physique Nucléaire et Corpusculaire, Faculté de Sciences, Université de Genève, 24 Quai Ernest Ansermet, Geneva; 1211, Switzerland;²⁰Institute of Frontier and Interdisciplinary Science, Shandong University, Shandong, Qingdao; 266237, China;²¹APC, Universite Paris Cite, CNRS, IN2P3, CEA/IRFU, Observatoire de Paris, Paris; 119 75205, France;²²Department of Engineering Physics, Tsinghua University, Beijing; 100084, China;²³School of Physics and Microelectronics, Zhengzhou University, Henan, Zhengzhou; 450001, China;²⁴Yunnan Observatories, Chinese Academy of Sciences, Yunnan, Kunming; 650216, China;²⁵College of Physics, Sichuan University, Sichuan, Chengdu; 610065, China;²⁶Institute for Nuclear Research of Russian Academy of Sciences, Moscow; 117312, Russia;²⁷Moscow Institute of Physics and Technology, Moscow; 141700, Russia;²⁸School of Physics, Peking University, Beijing; 100871, China;²⁹School of Physical Science and Technology, Guangxi University, Guangxi, Nanning; 530004, China;³⁰Department of Physics, Faculty of Science, Mahidol University, Bangkok; 10400, Thailand;³¹Center 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;³²National Space Science Center, Chinese Academy of Sciences, Beijing; 100190, China
【年份】2023
【摘要】 The diffuse Galactic γ-ray emission, mainly produced via interactions between cosmic rays and the diffuse interstellar medium, is a very important probe of the distribution, propagation, and interaction of cosmic rays in the Milky Way. In this work w...
【文献类型】期刊

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