Performance of the muon detector A under TIBET III array-Reference-Cited by-同舟云学术

Performance of the muon detector A under TIBET III array

Published:2013-02 Issue:2 Volume:37 Page:026001
ISSN:1674-1137
Container-title:Chinese Physics C
language:
Short-container-title:Chinese Phys. C

Author:

Liu Cheng,Bi Xiao-Jun,Chen Tian-Lu,Chen Wen-Yi,Cui Shu-Wang,Danzengluobu ,Ding Lin-Kai,Ding Xiao-Hong,Feng Cun-Feng,Feng Zhao-Yang,Feng Zhen-Yong,Gou Quan-Bu,Guo Hong-Wei,Guo Yi-Qing,He Hui-Hai,Hou Zheng-Tao,Hu Hai-Bing,Hu Hong-Bo,Huang Jing,Li Wan-Jie,Jia Huan-Yu,Jiang Long,Kang Ming-Ming,Le Gui-Ming,Lei Wen-Hua,Li Ai-Feng,Li Hai-Jin,Liu Jin-Sheng,Liu Mao-Yuan,Lu Hong,Meng Xian-Ru,Qian Xiang-Li,Qu Xiao-Bo,Tan You-Heng,Wang Hui,Wu Han-Rong,Shen Chang-Quan,Shen Pei-Ruo,Xue Liang,Yang Zhen,Yuan Ai-Fang,Zhai Liu-Ming,Zhang Hui-Min,Zhang Ji-Long,Zhang Xue-Yao,Zhang Yong,Zhang Yi,Zhang Ying,Zhou Xun-Xiu

Publisher

IOP Publishing

Subject

Astronomy and Astrophysics,Instrumentation,Nuclear and High Energy Physics

Link

https://iopscience.iop.org/article/10.1088/1674-1137/37/2/026001/pdf

Reference20 articles.

1. Observation of TeV gamma rays from the Crab nebula using the atmospheric Cerenkov imaging technique

2. The All‐Particle Spectrum of Primary Cosmic Rays in the Wide Energy Range from 1014to 1017eV Observed with the Tibet‐III Air‐Shower Array

3. Observation of Multi-T[CLC]e[/CLC]V Gamma Rays from the Crab Nebula using the Tibet Air Shower Array

4. Detection of Multi‐TeV Gamma Rays from Markarian 501 during an Unforeseen Flaring State in 1997 with the Tibet Air Shower Array

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