Physics – High Energy Physics – High Energy Physics - Experiment
Scientist
Physics
High Energy Physics
High Energy Physics - Experiment
Scientist
Minnesota, University, Minneapolis, MN
Department of Astronomy, Nanjing University, 22 Hankou Lu, Nanjing, Jiangsu 210093, China
The Tibet AS gamma Collaboration
The Tibet ASgamma Collaboration
Shandong University, Jinan, P. R. China
The ARGO-YBJ Collaboration
Department of Earth and Environmental Sciences, Rensselaer Polytechnic Institute, Troy, NY 12180, USA; Department of Geosciences, 1040 E. 4th Street, The University of Arizona, Tucson, AZ 85721, USA
Department of Physics, Shandong University, Jinan 250100, China
Department of Earth and Environmental Sciences, Rensselaer Polytechnic Institute, 110 8th Street, Jonsson-Rowland Science Center, Troy, NY 12180-3590, USA
Department of Physics, Shangdong University, Jinan 250100, China
Yunnan Astronomical Observatory, Chinese Academy of Sciences, Kunming 650011, China
CAWS, Chinese Academy of Meteorological Sciences, Beijing, China
State Key Laboratory of Space Weather, Chinese Academy of Sciences, Beijing, China
National Astronomical Observatoires / Yunnan Astronomical Observatory, Chinese Academy of Sciences
Beijing Observatory, People's Republic of China
Yunnan Astronomical Observatory, Chinese Academy of Sciences, Kunming 650011, China and National Astronomical Observatoires, Chinese Academy of Sciences Beijing 100012, China
Institute of Modern Physics, Chinese Academy of Sciences, Lanzhou 730000, People's Republic of China
Shangdong University, Jinan, China
Yunnan Astronomical Observatory, National Astronomical Observatoires, Chinese Academy of Sciences, Kunming, Yunnan 650011, China
0.35-3.5 micron photometry of polarized QSOs
0.35-3.5 micron photometry of X-ray emitting QSOs
6Li/7Li, 10B/11B and 7Li/11B/28Si in Individual Interplanetary Dust Particles
A large underground water Cherenkov muon detector array with the Tibet air shower array for Gamma-ray astronomy in the 100 TeV region: detector design and simulation
A large underground water Cherenkov muon detector array with the Tibet air shower array for the Gamma-ray astronomy in the 100 TeV region: Overview and physics goal
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