【作者】Aharonian, F.，An, Q.，Axikegu，Bai, L. X.，Bai, Y. X.，Bao, Y. W.，Bastieri, D.，Bi, X. J.，Bi, Y. J.，Cai, H.，Cai, J. T.，Cao, Z.，Cao, Z.，Chang, J.，Chang, J. F.，Chang, X. C.，Chen, B. M.，Chen, J.，Chen, L.，Chen, L.，Chen, L.，Chen, M. J.，Chen, M. L.，Chen, Q. H.，Chen, S. H.，Chen, S. Z.，Chen, T. L.，Chen, X. L.，Chen, Y.，Cheng, N.，Cheng, Y. D.，Cui, S. W.，Cui, X. H.，Cui, Y. D.，Dai, B. Z.，Dai, H. L.，Dai, Z. G.，Danzengluobu，della Volpe, D.，Piazzoli, B. D'Ettorre，Dong, X. J.，Fan, J. H.，Fan, Y. Z.，Fan, Z. X.
【作者单位】1 Chinese Acad Sci, Key Lab Particle Astrophy, Inst High Energy Phys, Beijing 100049, Peoples R China; 2 Chinese Acad Sci, Inst High Energy Phys, Expt Phys Div, Beijing 100049, Peoples R China; 3 Chinese Acad Sci, Comp Ctr, Inst High Energy Phys, Beijing 100049, Peoples R China; 4 Univ Chinese Acad Sci, Beijing 100049, Peoples R China; 5 TIANFU Cosm Ray Res Ctr, Chengdu, Sichuan, Peoples R China; 6 State Key Lab Particle Detect & Elect, Beijing, Peoples R China; 7 Univ Sci & Technol China, Hefei 230026, Anhui, Peoples R China; 8 Tsinghua Univ, Dept Engn Phys, Beijing 100084, Peoples R China; 9 Chinese Acad Sci, Natl Astron Observ, Beijing 100101, Peoples R China; 10 Chinese Acad Sci, Natl Space Sci Ctr, Beijing 100190, Peoples R China; 11 Peking Univ, Sch Phys, Beijing 100871, Peoples R China; 12 Guangzhou Univ, Ctr Astrophys, Guangzhou 510006, Guangdong, Peoples R China; 13 Sun Yat Sen Univ, Sch Phys & Astron, Zhuhai 519000, Guangdong, Peoples R China; 14 Sun Yat Sen Univ, Sch Phys Guangzhou, Zhuhai 519000, Guangdong, Peoples R China; 15 Guangxi Univ, Sch Phys Sci & Technol, Nanning 530004, Guangxi, Peoples R China; 16 Hebei Normal Univ, Shijiazhuang 050024, Hebei, Peoples R China; 17 Zhengzhou Univ, Sch Phys & Microelect, Zhengzhou 450001, Henan, Peoples R China; 18 Nanjing Univ, Sch Astron & Space Sci, Nanjing 210023, Jiangsu, Peoples R China; 19 Chinese Acad Sci, Purple Mt Observ, Key Lab Dark Matter & Space Astron, Nanjing 210023, Jiangsu, Peoples R China; 20 Shandong Univ, Inst Frontier & Interdisciplinary Sci, Qingdao 266237, Shandong, Peoples R China; 21 Chinese Acad Sci, Shanghai Astron Observ, Key Lab Res Galaxies & Cosmol, Shanghai 200030, Peoples R China; 22 Shanghai Jiao Tong Univ, Tsung Dao Lee Inst, Shanghai 200240, Peoples R China; 23 Shanghai Jiao Tong Univ, Sch Phys & Astron, Shanghai 200240, Peoples R China; 24 Southwest Jiaotong Univ, Sch Phys Sci & Technol, Chengdu 610031, Sichuan, Peoples R China; 25 Southwest Jiaotong Univ, Sch Informat Sci & Technol, Chengdu 610031, Sichuan, Peoples R China; 26 Sichuan Univ, Coll Phys, Chengdu 610065, Sichuan, Peoples R China; 27 Tibet Univ, Key Lab Cosm Rays, Minist Educ, Lhasa 850000, Peoples R China; 28 Wuhan Univ, Sch Phys & Technol, Wuhan 430072, Hubei, Peoples R China; 29 Yunnan Univ, Sch Phys & Astron, Kunming 650091, Yunnan, Peoples R China; 30 Chinese Acad Sci, Yunnan Observ, Kunming 650216, Yunnan, Peoples R China; 31 Dublin Inst Adv Studies, 31 Fitzwilliam Pl, Dublin 2, Ireland; 32 Max Planck Inst Nucl Phys, POB 103980, D-69029 Heidelberg, Germany; 33 Univ Napoli Federico II, Dipartimento Fis, Complesso Univ Monte St Angelo, Via Cinthia, I-80126 Naples, Italy; 34 Russian Acad Sci, Inst Nucl Res, Moscow 117312, Russia; 35 Moscow Inst Phys & Technol, Moscow 141700, Russia; 36 Univ Geneva, Fac Sci, Dept Phys Nucl & Corpusculaire, 24 Quai Ernest Ansermet, CH-1211 Geneva, Switzerland; 37 Mahidol Univ, Fac Sci, Dept Phys, Bangkok 10400, Thailand
【ISSN】2509-9930
【摘要】 Purpose The main scientific goal of LHAASO-WCDA is to survey gamma-ray sources with energy from 100 GeV to 30 TeV. To observe high-energy shower events, especially to measure the energy spectrum of cosmic rays from 100 TeV to 10 PeV, a dynamic range ...
