【作者单位】Dublin Institute for Advanced Studies;Max-Planck-Institut for Nuclear Physics,Germany;State Key Laboratory of Particle Detection and Electronics,State Key Laboratory of Particle Detection and Electronics;University of Science and Technology of China,Anhui;School of Physical Science and Technology & School of Information Science and Technology,Southwest Jiaotong University;College of Physics,Sichuan University;Experimental Physics Division & Computing Center,Institute of High Energy Physics,Chinese Academy of Sciences,Key Laboratory of Particle Astrophyics,Chinese Academy of Sciences;TIANFU Cosmic Ray Research Center;School of Astronomy and Space Science,Nanjing University;Center for Astrophysics,Guangzhou University;University of Chinese Academy of Sciences;School of Physics and Technology,Wuhan University;Purple Mountain Observatory,Chinese Academy of Sciences,Key Laboratory of Dark Matter and Space Astronomy,Chinese Academy of Sciences;Hebei Normal University,Hebei;Shanghai Astronomical Observatory,Chinese Academy of Sciences,Key Laboratory for Research in Galaxies and Cosmology,Chinese Academy of Sciences;Tibet University,Key Laboratory of Cosmic Rays,Ministry of Education;National Astronomical Observatories,Chinese Academy of Sciences;School of Physics and Astronomy & School of Physics (Guangzhou),Sun Yat-sen University;School of Physics and Astronomy,Yunnan University;Departement de Physique Nucleaire et Corpusculaire,Faculte de Sciences,Universite de Geneve;Dipartimento di Fisica dell'Universita di Napoli “Federico II”,Complesso Universitario di Monte Sant'Angelo;Institute of Frontier and Interdisciplinary Science,Shandong University;Department of Engineering Physics,Tsinghua University;School of Physics and Microelectronics,Zhengzhou University;Yunnan Observatories,Chinese Academy of Sciences;Institute for Nuclear Research of Russian Academy of Sciences,Russia;School of Physics,Peking University;School of Physical Science and Technology,Guangxi University;Tsung-Dao Lee Institute & School of Physics and Astronomy,Shanghai Jiao Tong University
【年份】2021
【卷号】第5卷
【期号】 第4期
【页码】520-530
【关键词】LHAASO-WCDA WCDA++ Water Cherenkov detector Performance
【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 ...