Zobrazeno 1 - 10
of 12
pro vyhledávání: '"Xiang-Li Qian"'
Autor:
Xiang-Li, Qian, Jin-Fan, Chang, Cun-Feng, Feng, Zhao-Yang, Feng, Quan-Bu, Gou, Yi-Qing, Guo, Hong-Bo, Hu, Cheng, Liu, Zheng, Wang, Liang, Xue, Xue-Yao, Zhang, Yi, Zhang
In ground-based extensive air shower experiments, the direction and energy are reconstructed by measuring the relative arrival time of secondary particles, and the energy they deposit. The measurement precision of the arrival time is crucial for dete
Externí odkaz:
http://arxiv.org/abs/1312.4624
A novel trigger algorithm for wide-field-of-view imaging atmospheric Cherenkov technique experiments
Publikováno v:
Nuclear Science and Techniques. 33
Autor:
Guang-Guang Xin, Yu-Hua Yao, Xiang-Li Qian, Cheng Liu, Qi Gao, Dan-Zeng Luo-Bu, You-Liang Feng, Quan-Bu Gou, Hong-Bo Hu, Hai-Jin Li, Mao-Yuan Liu, Wei Liu, Bing-Qiang Qiao, Zhen Wang, Yi Zhang, Hao Cai, Tian-Lu Chen, Yi-Qing Guo
The observation of very-high-energy (VHE, $\rm >10~GeV$) $\gamma$-ray emission from $\rm \gamma$-ray bursts (GRBs), especially in the prompt phase, will provide critical information for understanding many aspects of their nature including the physica
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::30decc30933f60cbbedc415b597101b6
http://arxiv.org/abs/2103.04381
http://arxiv.org/abs/2103.04381
Publikováno v:
Nucl.Sci.Tech.
Nucl.Sci.Tech., 2021, 32 (5), pp.51. ⟨10.1007/s41365-021-00882-2⟩
Nucl.Sci.Tech., 2021, 32 (5), pp.51. ⟨10.1007/s41365-021-00882-2⟩
As a proposed detector, the giant radio array for neutrino detection (GRAND) is primarily designed to discover and study the origin of ultra-high-energy cosmic rays, with ultra-high-energy neutrinos presenting the main method for detecting ultra-high
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::34644c31e972c8cdd48a0af59082f641
https://hal.archives-ouvertes.fr/hal-03249381
https://hal.archives-ouvertes.fr/hal-03249381
Publikováno v:
Nucl.Sci.Tech.
Nucl.Sci.Tech., 2021, 32 (1), pp.5. ⟨10.1007/s41365-020-00841-3⟩
Nucl.Sci.Tech., 2021, 32 (1), pp.5. ⟨10.1007/s41365-020-00841-3⟩
International audience; Neutrino detection in the 100 PeV energy region is the ultimate means of studying the origin of ultra-high-energy cosmic rays, in which the large radio detection array giant radio array for neutrino detection (GRAND) project a
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0128921027b8248397b6c2b5c1278d64
https://hal.archives-ouvertes.fr/hal-03136693
https://hal.archives-ouvertes.fr/hal-03136693
Autor:
Mao-Yuan Liu, C. Hou, Yi-Qing Guo, Tianlu Chen, Hui Cai, Y. Y. Guo, B. Q. Qiao, S. R. Zhang, Xiangdong Sheng, Xue-Yao Zhang, Hongbo Hu, Jia Liu, Quanbu Gou, Cheng Liu, Xiang-Li Qian, Yi Zhang, Zhen Wang, Danzengluobu, Zhen Tian, Youliang Feng, Qun Wang, Q. Gao, Liang Xue, Yuhua Yao, Jinfan Chang, Hai-Jin Li, Labaciren
Publikováno v:
Experimental Astronomy. 45:363-377
A scintillation detector array composed of 115 detectors and covering an area of about 20000 m2 was 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 el
Autor:
Wei-Min Liu, Na Wang, Xiang-Li Qian, Chun-wei Leng, Jian-Ping Yuan, Wen-Cong Chen, Long Jiang
Publikováno v:
Research in Astronomy and Astrophysics. 21:231
PSR J$1946+3417$ is a millisecond pulsar (MSP) with a spin period $P\simeq3.17\rm~ms$. Harbored in a binary with an orbital period $P_{\rm b}\simeq27$ days, the MSP is accompanied by a white dwarf (WD). The masses of the MSP and the WD were determine
Autor:
Yanhong Yu, Xiang-Li Qian, Yi Zhang, Xu Wang, Quanbu Gou, Cunfeng Feng, Wei Liu, Youliang Feng, Olivier Martineau-Huynh
Publikováno v:
Journal of Instrumentation
Journal of Instrumentation, IOP Publishing, 2021, 16 (04), pp.P04008. ⟨10.1088/1748-0221/16/04/P04008⟩
Journal of Instrumentation, IOP Publishing, 2021, 16 (04), pp.P04008. ⟨10.1088/1748-0221/16/04/P04008⟩
GRANDProto35 is the first stage of the GRAND project. It will be composed of an array of 35 radio antennas and 24 scintillation detectors in which the radio and scintillating subarrays will be triggered independently. The scintillation detector array
Autor:
Gui-Ming Le, Z. Y. Feng, X. R. Meng, Long Jiang, H. W. Guo, Hui-Min Zhang, Ai-Fang Yuan, You-Heng Tan, Zhaoyang Feng, Quanbu Gou, Hong-Bo Hu, Ai-Feng Li, Wen-Yi Chen, Danzengluobu, Xue-Yao Zhang, Yi-Qing Guo, Pei-Ruo Shen, Shuwang Cui, Tian-Lu Chen, Zheng-Tao Hou, Yong Zhang, L. M. Zhai, Xiao-Jun Bi, H. Lu, W. D. Li, Liang Xue, J. S. Liu, Huihai He, Xun-Xiu Zhou, Cheng Liu, Jing Huang, Yi Zhang, Ming-Ming Kang, Hui Wang, Xiang-Li Qian, Haibing Hu, X. B. Qu, Hai-Jin Li, Zhen Yang, Xiao-Hong Ding, Huan-Yu Jia, Chang-Quan Shen, L. K. Ding, Ying Zhang, Wen-Hua Lei, Mao-Yuan Liu, Cunfeng Feng, Ji-Long Zhang, Han-Rong Wu
Publikováno v:
Chinese Physics C. 37:035001
We study the sidereal and solar time modulation of multi-TeV cosmic rays using the east-west method with Tibet III air shower array data taken from November 1999 to December 2008. The statistics are twice the amount used in our previous paper. In thi
Autor:
Shuwang Cui, Gui-Ming Le, Danzengluobu, L. M. Zhai, H. Lu, Z. Y. Feng, Xiao-Jun Bi, Huan-Yu Jia, X. B. Qu, Hai-Jin Li, Wen-Yi Chen, Haibing Hu, X. R. Meng, Hui-Min Zhang, You-Heng Tan, Liang Xue, Ming-Ming Kang, Huihai He, Hui Wang, Xiang-Li Qian, Zheng-Tao Hou, Jing Huang, Zhaoyang Feng, Mao-Yuan Liu, Xun-Xiu Zhou, Zhen Yang, Yi-Qing Guo, Xiao-Hong Ding, Ji-Long Zhang, Han-Rong Wu, Xue-Yao Zhang, Cheng Liu, Ai-Fang Yuan, Pei-Ruo Shen, Ai-Feng Li, Yi Zhang, Yong Zhang, H. W. Guo, Tian-Lu Chen, Wen-Hua Lei, Quanbu Gou, J. S. Liu, W. D. Li, Long Jiang, Hong-Bo Hu, Chang-Quan Shen, L. K. Ding, Ying Zhang, Cunfeng Feng
Publikováno v:
Chinese Physics C. 37:026001
In order to observe gamma rays in the 100 TeV energy region, the 4500 m(2) underground muon detector array using water Cherenkov technique is constructed, forming the TIBET III+MD hybrid array. Because the showers induced by primary gamma rays contai