Performance of a scintillation detector array operated with LHAASO-KM2A electronics
Performance of a scintillation detector array operated with LHAASO-KM2A electronics
复制标题
使用 LHAASO-KM2A 电子设备操作的闪烁探测器阵列的性能
DOI:
10.1007/s10686-018-9588-z
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发表时间:
2018-04
影响因子:
3
通讯作者:
Y
中科院分区:
文献类型:
--
作者:
Wang Zhen;Guo Yiqing;Cai Hui;Chang Jinfan;Chen Tianlu;Danzengluobu;Feng Youliang;Gao Qi;Gou Quanbu;Guo Yingying;Hou Chao;Hu Hongbo;Labaciren;Liu Cheng;Li Haijin;Liu Jia;Liu Maoyuan;Qiao Bingqiang;Qian Xiangli;Sheng Xiangdong;Tian Zhen;Wang Qun;Xue Liang;Y
A scintillation detector array composed of 115 detectors and covering an area of about 20000 m2was installed at the end of 2016 at the Yangbajing international cosmic ray observatory and has been taking data since then. The array is equipped with electronics from Large High Altitude Air Shower Observatory Square Kilometer Complex Array (LHAASO-KM2A) and, in turn, currently serves as the largest debugging and testing platform for the LHAASO-KM2A. Furthermore, the array was used to study the performance of a wide field-of-view air Cherenkov telescope by providing accurate information on the shower core, direction and energy, etc. This work is mainly dealing with the scintillation detector array. The experimental setup and the offline calibration are described in detail. Then, a thorough comparison between the data and Monte Carlo (MC) simulations is presented and a good agreement is obtained. With the even-odd method, the resolutions of the shower direction and core are measured. Finally, successful observations of the expected Moon’s and Sun’s shadows of cosmic rays (CRs) verify the measured angular resolution.
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影响因子:
3.6
作者:
Yuan Ai-Fang;Zhai Liu-Ming;Zhang Hui-Min;Zhang Ji-Long;Zhang Xue-Yao;Zhang Yong;Zhang Yi;Zhang Ying;Zhou Xun-Xiu
通讯作者:
Zhou Xun-Xiu
影响因子:
4.9
作者:
Liu Ye;Cao Zhen;Chen Songzhan;Chen Yang;Cui Shuwang;He Huihai;Huang Xingtao;Ma Xinhua;Yuan Qiang;Zhang Xiao
通讯作者:
Zhang Xiao
DOI:
10.1088/1742-6596/120/6/062024
发表时间:
2008-07
期刊:
Journal of Physics: Conference Series
影响因子:
--
作者:
M. Amenomori;X. Bi;D. Chen;S. Cui;Danzengluobu;L. Ding;X. Ding;C. Fan;C. Feng;Zhaoyang Feng;Z. Feng;X. Gao;Q. Geng;H. Guo;Hao-Ning He;M. He;K. Hibino;N. Hotta;Haibing Hu;Haiming Hu;J. Huang;Q. Huang;H. Jia;F. Kajino;K. Kasahara;Y. Katayose;C. Kato;K. Kawata;Labaciren;G. Le;A. Li;J. Li;Y. Lou;H. Lu;Shan Lu;X. Meng;K. Mizutani;J. Mu;K. Munakata;A. Nagai;H. Nanjo;M. Nishizawa;M. Ohnishi;I. Ohta;H. Onuma;T. Ouchi;S. Ozawa;Jie Ren;T. Saito;T. Saito;M. Sakata;T. Sako;M. Shibata;A. Shiomi;T. Shirai;H. Sugimoto;M. Takita;Y. Tan;N. Tateyama;S. Torii;H. Tsuchiya;S. Udo;B. Wang;Hong Wang;X. Wang;Yusa Wang;Y. Wang;H. Wu;L. Xue;Y. Yamamoto;C. Yan;X. Yang;S. Yasue;Z. Ye;G. Yu;A. Yuan;T. Yuda;H. Zhang;J. Zhang;N. Zhang;X. Zhang;Y. Zhang;Zhaxisangzhu;X. Zhou
通讯作者:
M. Amenomori;X. Bi;D. Chen;S. Cui;Danzengluobu;L. Ding;X. Ding;C. Fan;C. Feng;Zhaoyang Feng;Z. Feng;X. Gao;Q. Geng;H. Guo;Hao-Ning He;M. He;K. Hibino;N. Hotta;Haibing Hu;Haiming Hu;J. Huang;Q. Huang;H. Jia;F. Kajino;K. Kasahara;Y. Katayose;C. Kato;K. Kawata;Labaciren;G. Le;A. Li;J. Li;Y. Lou;H. Lu;Shan Lu;X. Meng;K. Mizutani;J. Mu;K. Munakata;A. Nagai;H. Nanjo;M. Nishizawa;M. Ohnishi;I. Ohta;H. Onuma;T. Ouchi;S. Ozawa;Jie Ren;T. Saito;T. Saito;M. Sakata;T. Sako;M. Shibata;A. Shiomi;T. Shirai;H. Sugimoto;M. Takita;Y. Tan;N. Tateyama;S. Torii;H. Tsuchiya;S. Udo;B. Wang;Hong Wang;X. Wang;Yusa Wang;Y. Wang;H. Wu;L. Xue;Y. Yamamoto;C. Yan;X. Yang;S. Yasue;Z. Ye;G. Yu;A. Yuan;T. Yuda;H. Zhang;J. Zhang;N. Zhang;X. Zhang;Y. Zhang;Zhaxisangzhu;X. Zhou
DOI:
10.5445/ir/270043064
发表时间:
1998-02
期刊:
--
影响因子:
--
作者:
D. Heck;J. Knapp;J. Capdevielle;G. Schatz;T. Thouw
通讯作者:
D. Heck;J. Knapp;J. Capdevielle;G. Schatz;T. Thouw
影响因子:
1.3
作者:
Y. Zhang;Q.-B. Gou;H. Cai;T.-L. Chen;Danzengluobu;C.-F. Feng;Y.-L. Feng;Z.-Y. Feng;Q. Gao;X.-J. Gao;Y.-Q. Guo;Y.-Y. Guo;Y.-Y. Hou;H.-B. Hu;C. Jin;H.-J. Li;C. Liu;M.-Y. Liu;X.-L. Qian;Z. Tian;Z. Wang;L. Xue;X.-Y. Zhang;Xi-Ying Zhang
通讯作者:
Xi-Ying Zhang