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1. The First LHAASO Catalog of Gamma-Ray Sources

Author: Zhen Cao, F. Aharonian, Q. An, Axikegu, Y. X. Bai, Y. W. Bao, D. Bastieri, X. J. Bi, Y. J. Bi, J. T. Cai, Q. Cao, W. Y. Cao, Zhe Cao, J. Chang, J. F. Chang, A. M. Chen, E. S. Chen, Liang Chen, Lin Chen, Long Chen, M. J. Chen, M. L. Chen, Q. H. Chen, S. H. Chen, S. Z. Chen, T. L. Chen, Y. Chen, N. Cheng, Y. D. Cheng, M. Y. Cui, S. W. Cui, X. H. Cui, Y. D. Cui, B. Z. Dai, H. L. Dai, Z. G. Dai, Danzengluobu, D. della Volpe, X. Q. Dong, K. K. Duan, J. H. Fan, Y. Z. Fan, J. Fang, K. Fang, C. F. Feng, L. Feng, S. H. Feng, X. T. Feng, Y. L. Feng, S. Gabici, B. Gao, C. D. Gao, L. Q. Gao, Q. Gao, W. Gao, W. K. Gao, M. M. Ge, L. S. Geng, G. Giacinti, G. H. Gong, Q. B. Gou, M. H. Gu, F. L. Guo, X. L. Guo, Y. Q. Guo, Y. Y. Guo, Y. A. Han, H. H. He, H. N. He, J. Y. He, X. B. He, Y. He, M. Heller, Y. K. Hor, B. W. Hou, C. Hou, X. Hou, H. B. Hu, Q. Hu, S. C. Hu, D. H. Huang, T. Q. Huang, W. J. Huang, X. T. Huang, X. Y. Huang, Y. Huang, Z. C. Huang, X. L. Ji, H. Y. Jia, K. Jia, K. Jiang, X. W. Jiang, Z. J. Jiang, M. Jin, M. M. Kang, T. Ke, D. Kuleshov, K. Kurinov, B. B. Li, Cheng Li, Cong Li, D. Li, F. Li, H. B. Li, H. C. Li, H. Y. Li, J. Li, Jian Li, Jie Li, K. Li, W. L. Li, X. R. Li, Xin Li, Y. Z. Li, Zhe Li, Zhuo Li, E. W. Liang, Y. F. Liang, S. J. Lin, B. Liu, C. Liu, D. Liu, H. Liu, H. D. Liu, J. Liu, J. L. Liu, J. Y. Liu, M. Y. Liu, R. Y. Liu, S. M. Liu, W. Liu, Y. Liu, Y. N. Liu, R. Lu, Q. Luo, H. K. Lv, B. Q. Ma, L. L. Ma, X. H. Ma, J. R. Mao, Z. Min, W. Mitthumsiri, H. J. Mu, Y. C. Nan, A. Neronov, Z. W. Ou, B. Y. Pang, P. Pattarakijwanich, Z. Y. Pei, M. Y. Qi, Y. Q. Qi, B. Q. Qiao, J. J. Qin, D. Ruffolo, A. Sáiz, D. Semikoz, C. Y. Shao, L. Shao, O. Shchegolev, X. D. Sheng, F. W. Shu, H. C. Song, Yu. V. Stenkin, V. Stepanov, Y. Su, Q. N. Sun, X. N. Sun, Z. B. Sun, P. H. T. Tam, Q. W. Tang, Z. B. Tang, W. W. Tian, C. Wang, C. B. Wang, G. W. Wang, H. G. Wang, H. H. Wang, J. C. Wang, K. Wang, L. P. Wang, L. Y. Wang, P. H. Wang, R. Wang, W. Wang, X. G. Wang, X. Y. Wang, Y. Wang, Y. D. Wang, Y. J. Wang, Z. H. Wang, Z. X. Wang, Zhen Wang, Zheng Wang, D. M. Wei, J. J. Wei, Y. J. Wei, T. Wen, C. Y. Wu, H. R. Wu, S. Wu, X. F. Wu, Y. S. Wu, S. Q. Xi, J. Xia, J. J. Xia, G. M. Xiang, D. X. Xiao, G. Xiao, G. G. Xin, Y. L. Xin, Y. Xing, Z. Xiong, D. L. Xu, R. F. Xu, R. X. Xu, W. L. Xu, L. Xue, D. H. Yan, J. Z. Yan, T. Yan, C. W. Yang, F. Yang, F. F. Yang, H. W. Yang, J. Y. Yang, L. L. Yang, M. J. Yang, R. Z. Yang, S. B. Yang, Y. H. Yao, Z. G. Yao, Y. M. Ye, L. Q. Yin, N. Yin, X. H. You, Z. Y. You, Y. H. Yu, Q. Yuan, H. Yue, H. D. Zeng, T. X. Zeng, W. Zeng, M. Zha, B. B. Zhang, F. Zhang, H. M. Zhang, H. Y. Zhang, J. L. Zhang, L. X. Zhang, Li Zhang, P. F. Zhang, P. P. Zhang, R. Zhang, S. B. Zhang, S. R. Zhang, S. S. Zhang, X. Zhang, X. P. Zhang, Y. F. Zhang, Yi Zhang, Yong Zhang, B. Zhao, J. Zhao, L. Zhao, L. Z. Zhao, S. P. Zhao, F. Zheng, B. Zhou, H. Zhou, J. N. Zhou, M. Zhou, P. Zhou, R. Zhou, X. X. Zhou, C. G. Zhu, F. R. Zhu, H. Zhu, K. J. Zhu, X. Zuo, and (The LHAASO Collaboration)
Subjects: Gamma-ray astronomy, Gamma-ray observatories, Catalogs, Astrophysics, QB460-466
Abstract: We present the first catalog of very-high-energy and ultra-high-energy gamma-ray sources detected by the Large High Altitude Air Shower Observatory. The catalog was compiled using 508 days of data collected by the Water Cherenkov Detector Array from 2021 March to 2022 September and 933 days of data recorded by the Kilometer Squared Array from 2020 January to 2022 September. This catalog represents the main result from the most sensitive large coverage gamma-ray survey of the sky above 1 TeV, covering decl. from −20° to 80°. In total, the catalog contains 90 sources with an extended size smaller than 2° and a significance of detection at >5 σ . Based on our source association criteria, 32 new TeV sources are proposed in this study. Among the 90 sources, 43 sources are detected with ultra-high energy ( E > 100 TeV) emission at >4 σ significance level. We provide the position, extension, and spectral characteristics of all the sources in this catalog.
Published: 2024
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2. Construction and on-site performance of the LHAASO WFCTA camera

Author: F. Aharonian, Q. An, Axikegu, L. X. Bai, Y. X. Bai, Y. W. Bao, D. Bastieri, X. J. Bi, Y. J. Bi, H. Cai, J. T. Cai, Z. Cao, J. Chang, J. F. Chang, X. C. Chang, B. M. Chen, J. Chen, L. Chen, M. J. Chen, M. L. Chen, Q. H. Chen, S. H. Chen, S. Z. Chen, T. L. Chen, X. L. Chen, Y. Chen, N. Cheng, Y. D. Cheng, S. W. Cui, X. H. Cui, Y. D. Cui, B. Z. Dai, H. L. Dai, Z. G. Dai, Danzengluobu, D. della Volpe, B. D’Ettorre Piazzoli, X. J. Dong, J. H. Fan, Y. Z. Fan, Z. X. Fan, J. Fang, K. Fang, C. F. Feng, L. Feng, S. H. Feng, Y. L. Feng, B. Gao, C. D. Gao, Q. Gao, W. Gao, M. M. Ge, L. S. Geng, G. H. Gong, Q. B. Gou, M. H. Gu, J. G. Guo, X. L. Guo, Y. Q. Guo, Y. Y. Guo, Y. A. Han, H. H. He, H. N. He, J. C. He, S. L. He, X. B. He, Y. He, M. Heller, Y. K. Hor, C. Hou, X. Hou, H. B. Hu, S. Hu, S. C. Hu, X. J. Hu, D. H. Huang, Q. L. Huang, W. H. Huang, X. T. Huang, Z. C. Huang, F. Ji, X. L. Ji, H. Y. Jia, K. Jiang, Z. J. Jiang, C. Jin, D. Kuleshov, K. Levochkin, B. B. Li, C. Li, F. Li, H. B. Li, H. C. Li, H. Y. Li, J. Li, K. Li, W. L. Li, X. Li, X. R. Li, Y. Li, Y. Z. Li, Z. Li, E. W. Liang, Y. F. Liang, S. J. Lin, B. Liu, C. Liu, D. Liu, H. Liu, H. D. Liu, J. Liu, J. L. Liu, J. S. Liu, J. Y. Liu, M. Y. Liu, R. Y. Liu, S. M. Liu, W. Liu, Y. N. Liu, Z. X. Liu, W. J. Long, R. Lu, H. K. Lv, B. Q. Ma, L. L. Ma, X. H. Ma, J. R. Mao, A. Masood, W. Mitthumsiri, T. Montaruli, Y. C. Nan, B. Y. Pang, P. Pattarakijwanich, Z. Y. Pei, M. Y. Qi, D. Ruffolo, V. Rulev, A. Sáiz, L. Shao, O. Shchegolev, X. D. Sheng, J. R. Shi, H. C. Song, Yu. V. Stenkin, V. Stepanov, Q. N. Sun, X. N. Sun, Z. B. Sun, P. H. T. Tam, Z. B. Tang, W. W. Tian, B. D. Wang, C. Wang, H. Wang, H. G. Wang, J. C. Wang, J. S. Wang, L. P. Wang, L. Y. Wang, R. N. Wang, W. Wang, X. G. Wang, X. J. Wang, X. Y. Wang, Y. D. Wang, Y. J. Wang, Y. P. Wang, Z. Wang, Z. H. Wang, Z. X. Wang, D. M. Wei, J. J. Wei, Y. J. Wei, T. Wen, C. Y. Wu, H. R. Wu, S. Wu, W. X. Wu, X. F. Wu, S. Q. Xi, J. Xia, J. J. Xia, G. M. Xiang, G. Xiao, H. B. Xiao, G. G. Xin, Y. L. Xin, Y. Xing, D. L. Xu, R. X. Xu, L. Xue, D. H. Yan, C. W. Yang, F. F. Yang, J. Y. Yang, L. L. Yang, M. J. Yang, R. Z. Yang, S. B. Yang, Y. H. Yao, Z. G. Yao, Y. M. Ye, L. Q. Yin, N. Yin, X. H. You, Z. Y. You, Y. H. Yu, Q. Yuan, H. D. Zeng, T. X. Zeng, W. Zeng, Z. K. Zeng, M. Zha, X. X. Zhai, B. B. Zhang, H. M. Zhang, H. Y. Zhang, J. L. Zhang, J. W. Zhang, L. Zhang, L. X. Zhang, P. F. Zhang, P. P. Zhang, R. Zhang, S. R. Zhang, S S. Zhang, X. Zhang, X. P. Zhang, Y. Zhang, Y. F. Zhang, Y. L. Zhang, B. Zhao, J. Zhao, L. Zhao, L. Z. Zhao, S. P. Zhao, F. Zheng, Y. Zheng, B. Zhou, H. Zhou, J. N. Zhou, P. Zhou, R. Zhou, X. X. Zhou, C. G. Zhu, F. R. Zhu, H. Zhu, K. J. Zhu, X. Zuo, and The LHAASO Collaboration
Subjects: Astrophysics, QB460-466, Nuclear and particle physics. Atomic energy. Radioactivity, QC770-798
Abstract: Abstract The focal plane camera is the core component of the Wide Field-of-view Cherenkov/fluorescence Telescope Array (WFCTA) of the Large High-Altitude Air Shower Observatory (LHAASO). Because of the capability of working under moonlight without aging, silicon photomultipliers (SiPM) have been proven to be not only an alternative but also an improvement to conventional photomultiplier tubes (PMT) in this application. Eighteen SiPM-based cameras with square light funnels have been built for WFCTA. The telescopes have collected more than 100 million cosmic ray events and preliminary results indicate that these cameras are capable of working under moonlight. The characteristics of the light funnels and SiPMs pose challenges (e.g. dynamic range, dark count rate, assembly techniques). In this paper, we present the design features, manufacturing techniques and performances of these cameras. Finally, the test facilities, the test methods and results of SiPMs in the cameras are reported here.
Published: 2021
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3. Line-of-shower trigger method to lower energy threshold for GRB detection using LHAASO-WCDA

Author: C. F. Feng, Bin Zhou, X. L. Ji, R. Lu, H. B. Xiao, J. R. Shi, W. Zeng, Z. H. Wang, Shengxue Zhang, Pak-Hin Thomas Tam, H. C. Li, Jun Liu, H. Y. Jia, B. D'Ettorre Piazzoli, W. X. Wu, Junjie Mao, Y. Q. Guo, Dong Liu, F. Ji, H. R. Wu, Y. J. Wei, Alejandro Sáiz, Oleg Shchegolev, L. Feng, V. Rulev, L. Xue, Xuliang Chen, Xing-Yuan Hou, D. M. Wei, S. Hu, M. L. Chen, Jianeng Zhou, J. Y. Liu, Warit Mitthumsiri, Y. Zhang, Q. An, Y. He, Q. Gao, Ruizhi Yang, X. N. Sun, H. B. Hu, H. Liu, L. Chen, X. G. Wang, S. Q. Xi, J. Fang, X. H. You, Ping Zhou, Z. C. Huang, Y. Z. Li, P. F. Zhang, C. Y. Wu, Hong-Guang Wang, G. M. Xiang, W. Liu, Yu-Lei Chen, Zihuang Cao, X. C. Chang, Z. K. Zeng, Y. J. Bi, H. D. Liu, Y. D. Cheng, Bo Zhang, Y. Zheng, L. Q. Yin, Duo Yan, F. Zheng, Hao Zhou, X. X. Zhou, Q. Yuan, Hefan Li, J. F. Chang, Z. X. Liu, Felix Aharonian, H. N. He, C. D. Gao, Lei Zhao, Q. H. Chen, Youping Li, Y. M. Ye, B. B. Li, Yongchun Wang, Y. D. Cui, Bai Yibing, L. P. Wang, J. B. Zhao, Y. J. Wang, J. Y. Yang, S. Z. Chen, Yunchao Liu, B. Z. Dai, Rong Xu, Z. X. Fan, Z. Y. You, Z. G. Dai, X. F. Wu, He Zhang, S. H. Feng, S. B. Yang, J. J. Xia, W. Gao, S. L. He, Y. P. Wang, B. M. Chen, Fan Yang, A. Masood, Kun Fang, S.H. Chen, Yugang Zhang, H. Cai, Lang Shao, H. Wang, J.W. Xia, L. Z. Zhao, G. C. Xiao, X. X. Zhai, Y. C. Nan, Shi-Qi Hu, X. J. Bi, Z. Li, R. Liu, E. W. Liang, X. Zuo, M. J. Yang, Y. H. Yao, W. L. Li, L. X. Zhang, H. K. Lv, Xufang Li, B. Y. Pang, Zebo Tang, M. H. Gu, Z. Y. Pei, Xuejiao Li, F. R. Zhu, T. L. Chen, Qie Sun, K. J. Zhu, Ying Zhang, H. M. Zhang, J. Chen, H. L. Dai, Y. L. Xin, T. Wen, S. W. Cui, M. Zha, J. C. He, W. H. Huang, L. X. Bai, Binyu Zhao, Yun-Feng Liang, Jixia Li, X. H. Cui, Xinbo He, K. Jiang, X. J. Hu, J. W. Zhang, Li-Sheng Geng, Wenwu Tian, Z. X. Wang, Xiaofei Zhang, David Ruffolo, Yu. V. Stenkin, C. Hou, Z. B. Sun, Shuibin Lin, Lu Zhang, K. Levochkin, Cheng Guang Zhu, X. D. Sheng, Minghao Qi, Houdun Zeng, Jun-Jie Wei, Jia Zhang, Y. A. Han, H. B. Li, Danzengluobu, Rui Zhang, H. C. Song, Linbin Yang, Y. Z. Fan, J. T. Cai, H. H. He, Y. M. Xing, F. Y. Li, D. H. Huang, H. Zhu, Xiang Zhang, M. M. Ge, J. G. Guo, S. R. Zhang, N. Cheng, L. L. Ma, G. H. Gong, J. S. Wang, Cunguo Wang, Shujuan Liu, N. Yin, Y. H. Yu, W. J. Long, Axikegu, Xuelong Wang, P. P. Zhang, Chunlong Li, Minghui Liu, D. Bastieri, Jinyao Liu, Z. G. Yao, X. H. Ma, M. Heller, K. Li, Z. J. Jiang, J. Liu, R. N. Wang, V. I. Stepanov, Jian Wang, Chiming Jin, D.A. Kuleshov, G. G. Xin, M. J. Chen, S. P. Zhao, Y. Y. Guo, Donglian Xu, X. L. Guo, X. J. Dong, Y. K. Hor, T. Montaruli, Y. L. Feng, W. Wang, P. Pattarakijwanich, S. Wu, B. D. Wang, C. X. Liu, Y. W. Bao, X. T. Huang, R. Zhou, L. Y. Wang, D. della Volpe, C. W. Yang, Jun-Hui Fan, Zujian Wang, Q. B. Gou, Qizhi Huang, B. Liu, Bingshui Gao, Xiang-Yu Wang, Tao Zeng, and Bin Ma
Subjects: Physics, Nuclear and High Energy Physics, Cherenkov detector, Astrophysics::High Energy Astrophysical Phenomena, Detector, Astrophysics, law.invention, Air shower, Nuclear Energy and Engineering, Duty cycle, law, Observatory, Gamma-ray burst, Energy (signal processing), Line (formation)
Abstract: Observation of high energy and very high emission from Gamma Ray Bursts (GRBs) is crucial to study the gigantic explosion and the underline processes. With a large field-of-view and almost full duty cycle, the Water Cherenkov Detector Array (WCDA), a sub-array of the Large High Altitude Air Shower Observatory (LHAASO), is appropriate to monitor the very high energy emission from unpredictable transients such as GRBs. Nevertheless, the main issue for an extensive air shower array is the high energy threshold which limits the horizon of the detector. To address this issue a new trigger method is developed in this article to lower the energy threshold of WCDA for GRB observation. The proposed method significantly improves the detection efficiency of WCDA for gamma-rays around the GRB direction at 10-300 GeV. The sensitivity of the WCDA for GRB detection with the new trigger method is estimated. The achieved sensitivity of the quarter WCDA array above 10 GeV is comparable with that of Fermi-LAT. The data analysis process and corresponding fluence upper limit for GRB 190719C is presented as an example.
Published: 2021

4. A dynamic range extension system for LHAASO WCDA-1

Author: F. Aharonian, Q. An, null Axikegu, L. X. Bai, Y. X. Bai, Y. W. Bao, D. Bastieri, X. J. Bi, Y. J. Bi, H. Cai, J. T. Cai, Z. Cao, J. Chang, J. F. Chang, X. C. Chang, B. M. Chen, J. Chen, L. Chen, M. J. Chen, M. L. Chen, Q. H. Chen, S. H. Chen, S. Z. Chen, T. L. Chen, X. L. Chen, Y. Chen, N. Cheng, Y. D. Cheng, S. W. Cui, X. H. Cui, Y. D. Cui, B. Z. Dai, H. L. Dai, Z. G. Dai, null Danzengluobu, D. della Volpe, B. D’Ettorre Piazzoli, X. J. Dong, J. H. Fan, Y. Z. Fan, Z. X. Fan, J. Fang, K. Fang, C. F. Feng, L. Feng, S. H. Feng, Y. L. Feng, B. Gao, C. D. Gao, Q. Gao, W. Gao, M. M. Ge, L. S. Geng, G. H. Gong, Q. B. Gou, M. H. Gu, J. G. Guo, X. L. Guo, Y. Q. Guo, Y. Y. Guo, Y. A. Han, H. H. He, H. N. He, J. C. He, S. L. He, X. B. He, Y. He, M. Heller, Y. K. Hor, C. Hou, X. Hou, H. B. Hu, S. Hu, S. C. Hu, X. J. Hu, D. H. Huang, Q. L. Huang, W. H. Huang, X. T. Huang, Y. Huang, Z. C. Huang, F. Ji, X. L. Ji, H. Y. Jia, K. Jiang, Z. J. Jiang, C. Jin, D. Kuleshov, K. Levochkin, B. B. Li, C. Li, F. Li, H. B. Li, H. C. Li, H. Y. Li, J. Li, K. Li, W. L. Li, X. Li, X. R. Li, Y. Li, Y. Z. Li, Z. Li, E. W. Liang, Y. F. Liang, S. J. Lin, B. Liu, C. Liu, D. Liu, H. Liu, H. D. Liu, J. Liu, J. L. Liu, J. S. Liu, J. Y. Liu, M. Y. Liu, R. Y. Liu, S. M. Liu, W. Liu, Y. N. Liu, Z. X. Liu, W. J. Long, R. Lu, H. K. Lv, B. Q. Ma, L. L. Ma, X. H. Ma, J. R. Mao, A. Masood, W. Mitthumsiri, T. Montaruli, Y. C. Nan, B. Y. Pang, P. Pattarakijwanich, Z. Y. Pei, M. Y. Qi, D. Ruffolo, V. Rulev, A. Sáiz, L. Shao, O. Shchegolev, X. D. Sheng, J. R. Shi, H. C. Song, Yu. V. Stenkin, V. Stepanov, Q. N. Sun, X. N. Sun, Z. B. Sun, P. H. T. Tam, Z. B. Tang, W. W. Tian, B. D. Wang, C. Wang, H. Wang, H. G. Wang, J. C. Wang, J. S. Wang, L. P. Wang, L. Y. Wang, R. N. Wang, W. Wang, X. G. Wang, X. J. Wang, X. Y. Wang, Y. D. Wang, Y. J. Wang, Y. P. Wang, Z. Wang, Z. H. Wang, Z. X. Wang, D. M. Wei, J. J. Wei, Y. J. Wei, T. Wen, C. Y. Wu, H. R. Wu, S. Wu, W. X. Wu, X. F. Wu, S. Q. Xi, J. Xia, J. J. Xia, G. M. Xiang, G. Xiao, H. B. Xiao, G. G. Xin, Y. L. Xin, Y. Xing, D. L. Xu, R. X. Xu, L. Xue, D. H. Yan, C. W. Yang, F. F. Yang, J. Y. Yang, L. L. Yang, M. J. Yang, R. Z. Yang, S. B. Yang, Y. H. Yao, Z. G. Yao, Y. M. Ye, L. Q. Yin, N. Yin, X. H. You, Z. Y. You, Y. H. Yu, Q. Yuan, H. D. Zeng, T. X. Zeng, W. Zeng, Z. K. Zeng, M. Zha, X. X. Zhai, B. B. Zhang, H. M. Zhang, H. Y. Zhang, J. L. Zhang, J. W. Zhang, L. Zhang, L. X. Zhang, P. F. Zhang, P. P. Zhang, R. Zhang, S. R. Zhang, S. S. Zhang, X. Zhang, X. P. Zhang, Y. Zhang, Y. F. Zhang, Y. L. Zhang, B. Zhao, J. Zhao, L. Zhao, L. Z. Zhao, S. P. Zhao, F. Zheng, Y. Zheng, B. Zhou, H. Zhou, J. N. Zhou, P. Zhou, R. Zhou, X. X. Zhou, C. G. Zhu, F. R. Zhu, H. Zhu, K. J. Zhu, and X. Zuo
Subjects: Physics, Nuclear and High Energy Physics, Physics::Instrumentation and Detectors, Dynamic range, Astrophysics::High Energy Astrophysical Phenomena, Astrophysics::Instrumentation and Methods for Astrophysics, Cosmic ray, Extension (predicate logic), Measure (mathematics), Effective nuclear charge, Nuclear physics, Air shower, Nuclear Energy and Engineering, Orders of magnitude (time), Energy (signal processing)
Abstract: 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 extension system (WCDA++) is designed to use a 1.5-inch PMT with a dynamic range of four orders of magnitude for each cell in WCDA-1. The dynamic range is extended by using these PMTs to measure the effective charge density in the core region of air shower events, which is an important parameter for identifying the composition of primary particles. The system has been running for more than one year. In this paper, the details of the design and performance of WCDA++ are presented.
Published: 2021

5. Constraints on heavy decaying dark matter from 570 days of LHAASO observations

Author: Zhen, Cao, F, Aharonian, Q, An, Axikegu, L X, Bai, Y X, Bai, Y W, Bao, D, Bastieri, X J, Bi, Y J, Bi, J T, Cai, Zhe, Cao, J, Chang, J F, Chang, E S, Chen, Liang, Chen, Long, Chen, M J, Chen, M L, Chen, Q H, Chen, S H, Chen, S Z, Chen, T L, Chen, Y, Chen, H L, Cheng, N, Cheng, Y D, Cheng, S W, Cui, X H, Cui, Y D, Cui, B, D'Ettorre Piazzoli, B Z, Dai, H L, Dai, Z G, Dai, Danzengluobu, D, Della Volpe, K K, Duan, J H, Fan, Y Z, Fan, Z X, Fan, J, Fang, K, Fang, C F, Feng, L, Feng, S H, Feng, X T, Feng, Y L, Feng, B, Gao, C D, Gao, L Q, Gao, Q, Gao, W, Gao, W K, Gao, M M, Ge, L S, Geng, G H, Gong, Q B, Gou, M H, Gu, F L, Guo, J G, Guo, X L, Guo, Y Q, Guo, Y Y, Guo, Y A, Han, H H, He, H N, He, S L, He, X B, He, Y, He, M, Heller, Y K, Hor, C, Hou, X, Hou, H B, Hu, Q, Hu, S, Hu, S C, Hu, X J, Hu, D H, Huang, W H, Huang, X T, Huang, X Y, Huang, Y, Huang, Z C, Huang, X L, Ji, H Y, Jia, K, Jia, K, Jiang, Z J, Jiang, M, Jin, M M, Kang, T, Ke, D, Kuleshov, K, Levochkin, B B, Li, Cheng, Li, Cong, Li, F, Li, H B, Li, H C, Li, H Y, Li, J, Li, Jian, Li, Jie, Li, K, Li, W L, Li, X R, Li, Xin, Li, Y Z, Li, Zhe, Li, Zhuo, Li, E W, Liang, Y F, Liang, S J, Lin, B, Liu, C, Liu, D, Liu, H, Liu, H D, Liu, J, Liu, J L, Liu, J S, Liu, J Y, Liu, M Y, Liu, R Y, Liu, S M, Liu, W, Liu, Y, Liu, Y N, Liu, W J, Long, R, Lu, Q, Luo, H K, Lv, B Q, Ma, L L, Ma, X H, Ma, J R, Mao, A, Masood, Z, Min, W, Mitthumsiri, Y C, Nan, Z W, Ou, B Y, Pang, P, Pattarakijwanich, Z Y, Pei, M Y, Qi, Y Q, Qi, B Q, Qiao, J J, Qin, D, Ruffolo, A, Sáiz, C Y, Shao, L, Shao, O, Shchegolev, X D, Sheng, J Y, Shi, H C, Song, Yu V, Stenkin, V, Stepanov, Y, Su, Q N, Sun, X N, Sun, Z B, Sun, P H T, Tam, Z B, Tang, W W, Tian, B D, Wang, C, Wang, H, Wang, H G, Wang, J C, Wang, J S, Wang, L P, Wang, L Y, Wang, R, Wang, R N, Wang, W, Wang, X G, Wang, X Y, Wang, Y, Wang, Y D, Wang, Y J, Wang, Y P, Wang, Z H, Wang, Z X, Wang, Zhen, Wang, Zheng, Wang, D M, Wei, J J, Wei, Y J, Wei, T, Wen, C Y, Wu, H R, Wu, S, Wu, X F, Wu, Y S, Wu, S Q, Xi, J, Xia, J J, Xia, G M, Xiang, D X, Xiao, G, Xiao, G G, Xin, Y L, Xin, Y, Xing, Z, Xiong, D L, Xu, R X, Xu, L, Xue, D H, Yan, J Z, Yan, C W, Yang, F F, Yang, H W, Yang, J Y, Yang, L L, Yang, M J, Yang, R Z, Yang, S B, Yang, Y H, Yao, Z G, Yao, Y M, Ye, L Q, Yin, N, Yin, X H, You, Z Y, You, Y H, Yu, Q, Yuan, H, Yue, H D, Zeng, T X, Zeng, W, Zeng, Z K, Zeng, M, Zha, X X, Zhai, B B, Zhang, F, Zhang, H M, Zhang, H Y, Zhang, J L, Zhang, L X, Zhang, Li, Zhang, Lu, Zhang, P F, Zhang, P P, Zhang, R, Zhang, S B, Zhang, S R, Zhang, S S, Zhang, X, Zhang, X P, Zhang, Y F, Zhang, Y L, Zhang, Yi, Zhang, Yong, Zhang, B, Zhao, J, Zhao, L, Zhao, L Z, Zhao, S P, Zhao, F, Zheng, Y, Zheng, B, Zhou, H, Zhou, J N, Zhou, P, Zhou, R, Zhou, X X, Zhou, C G, Zhu, F R, Zhu, H, Zhu, K J, Zhu, X, Zuo, S, Ando, M, Chianese, D F G, Fiorillo, G, Miele, K C Y, Ng, and GRAPPA (ITFA, IoP, FNWI)
Subjects: High Energy Astrophysical Phenomena (astro-ph.HE), High Energy Physics - Phenomenology, Cosmology and Nongalactic Astrophysics (astro-ph.CO), High Energy Physics - Phenomenology (hep-ph), General Physics and Astronomy, FOS: Physical sciences, Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: The kilometer square array (KM2A) of the large high altitude air shower observatory (LHAASO) aims at surveying the northern γ-ray sky at energies above 10 TeV with unprecedented sensitivity. γ-ray observations have long been one of the most powerful tools for dark matter searches, as, e.g., high-energy γ rays could be produced by the decays of heavy dark matter particles. In this Letter, we present the first dark matter analysis with LHAASO-KM2A, using the first 340 days of data from 1/2-KM2A and 230 days of data from 3/4-KM2A. Several regions of interest are used to search for a signal and account for the residual cosmic-ray background after γ/hadron separation. We find no excess of dark matter signals, and thus place some of the strongest γ-ray constraints on the lifetime of heavy dark matter particles with mass between 105 and 109 GeV. Our results with LHAASO are robust, and have important implications for dark matter interpretations of the diffuse astrophysical high-energy neutrino emission.
Published: 2022

6. Erratum: Quasi-elastic scattering of C10,11 and B10 from a Pbnat target [Phys. Rev. C 90 , 014606 (2014)]

Author: Y. Y. Yang, J. S. Wang, Q. Wang, D. Y. Pang, J. B. Ma, M. R. Huang, P. Ma, S. L. Jin, J. L. Han, Z. Bai, L. Jin, J. B. Chen, Q. Hu, R. Wada, S. Mukherjee, Z. Y. Sun, R. F. Chen, X. Y. Zhang, Z. G. Hu, X. H. Yuan, S. W. Xu, S. Z. Chen, X. G. Lei, L. X. Liu, W. H. Ma, S. T. Wang, D. Yan, X. H. Zhang, M. H. Zhao, Y. Zhou, Y. J. Zhou, Z. Y. Guo, Y. H. Zhang, H. S. Xu, and G. Q. Xiao
Published: 2022

7. [Hyper-IgE syndrome in adults characterized by disseminated mixed infection: a case report and literature review]

Author: M Z, Qiu, H, Zhang, D, Wu, R C, Chen, S Z, Chen, and L W, Wang
Subjects: Adult, Male, STAT3 Transcription Factor, Young Adult, Adolescent, Talaromyces, Coinfection, Humans, Immunoglobulin E, Job Syndrome, Retrospective Studies
Published: 2022

8. Role of surfactant molecular weight on morphology and properties of functionalized graphite oxide filled polypropylene nanocomposites

Author: Y. Wang, J-C. Wang, and S-Z. Chen
Subjects: Nanocomposites, graphite oxide, maleated polypropylene, functionalization, Materials of engineering and construction. Mechanics of materials, TA401-492, Chemical technology, TP1-1185
Abstract: Various surfactants of different molecular weights, including alkylamine, poly(oxypropylene) diamine (POP), and maleic anhydride grafted polypropylene (PPgMA) oligomers, were used for simultaneous funtionalization and reduction of graphite oxide (fGO). In this study, the effect of molecular weight and compatibility of the surfactants on the morphology and properties of the nanocomposites are reported. Wide-angle X-ray diffraction (WAXD) exhibited a definite interlayer thickness for GOA (alkylamine intercalated GO), however, the diffraction peaks were nearly suppressed for fGOs combining ODA with either POP (GOAP) or PPgMA (GOAE). The uniform dispersion of the fGO flakes in the polypropylene matrix resulted in the significant increase in both the degradation temperature and the crystallization temperature. A single characteristic melting peak of monoclinic (α) crystalline phase was observed from DSC traces, which was consistent with WAXD results. Dynamic mechanical analysis clearly indicated increase in both the storage modulus and the glass transition temperature of the nanocomposites due to the enhanced affinity between fGO and the polypropylene matrix. However, GOAP composite showed lower E' and Tg than GOAE because POP is less compatible with the matrix than PPgMA oligomer. Dielectric analysis also showed significant increase in both dielectric permittivity and dielectric loss at low frequency regimes with GOAE showing maximum dielectric properties. The finely dispersed GOAE and its compatibility with polymer matrix manifested the interfacial polarization, which gave rise to much greater ε' and ε" than other nanocomposites.
Published: 2014
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9. Ultrahigh-energy photons up to 1.4 petaelectronvolts from 12 γ-ray Galactic sources

Author: Alejandro Sáiz, Y. H. Yao, W. X. Wu, P. P. Zhang, Zhuo Li, R. Liu, Pak-Hin Thomas Tam, H. C. Li, Liang Chen, J. C. Wang, Y. L. Xin, L. Chen, M. J. Chen, Hong-Guang Wang, Y. J. Wei, S. Hu, Junjie Mao, Y. Q. Guo, J. Y. Liu, V. Rulev, P. F. Zhang, L. Xue, H. B. Hu, H. Liu, Rui Zhang, Linbin Yang, C. F. Feng, F. Ji, Xiaofei Zhang, F. Zheng, V. I. Stepanov, Ping Zhou, Q. H. Chen, H. R. Wu, Warit Mitthumsiri, X. C. Chang, Z. K. Zeng, C. D. Gao, Bin Zhou, W. L. Li, S. Z. Chen, M. M. Ge, Lei Zhao, Y. Z. Li, Y. Y. Guo, Y. J. Bi, Zhe Cao, Y. K. Hor, Xuejiao Li, H. D. Liu, S. H. Feng, B. Liu, Y. D. Cheng, Bo Zhang, H. K. Lv, H. M. Zhang, K. Levochkin, Y. J. Wang, L. X. Bai, Jixia Li, T. Montaruli, Duo Yan, Hefan Li, Ying Zhang, Bingshui Gao, Q. An, H. B. Xiao, J. R. Shi, X. D. Sheng, Z. X. Liu, W. H. Huang, M. L. Chen, Jianeng Zhou, Q. Gao, Minghao Qi, W. Zeng, Li-Sheng Geng, J. Chen, B. M. Chen, T. Wen, S. W. Cui, Z. X. Wang, Chiming Jin, S. B. Yang, L. Z. Zhao, C. W. Yang, J. B. Zhao, D.A. Kuleshov, Y. M. Xing, L. P. Wang, E. W. Liang, X. F. Wu, Zhe Li, B. Y. Pang, B. B. Li, X. Zuo, Cong Li, S. Q. Xi, Kun Fang, W. Gao, B. Z. Dai, Z. H. Wang, H. Cai, Jun Liu, Zhen Wang, J. C. He, Houdun Zeng, J. Fang, G. C. Xiao, Y. C. Nan, Z. G. Yao, Z. Y. Pei, Jun-Hui Fan, X. X. Zhou, Q. Yuan, H. B. Li, Shi-Qi Hu, G. G. Xin, J. F. Chang, Xufang Li, Oleg Shchegolev, G. M. Xiang, S. P. Zhao, W. Liu, X. L. Ji, M. J. Yang, H. H. He, R. Lu, Zhengguo Cao, Felix Aharonian, J. W. Zhang, H. C. Song, Yongchun Wang, Yugang Zhang, Wenwu Tian, He Zhang, Bai Yibing, S. L. He, Donglian Xu, Y. L. Feng, Zebo Tang, X. L. Guo, Y. D. Cui, X. J. Dong, Zheng Wang, Jun-Jie Wei, Q. B. Gou, Qizhi Huang, H. N. He, K. J. Zhu, M. Zha, B. D. Wang, Ruizhi Yang, X. N. Sun, Y. P. Wang, Z. C. Huang, H. L. Dai, H. Wang, Xiang Zhang, Xing-Yuan Hou, Yunchao Liu, H. Y. Jia, D. M. Wei, Z. G. Dai, Rong Xu, Fan Yang, A. Masood, F. Y. Li, Xinbo He, Youping Li, X. T. Huang, L. Y. Wang, X. R. Li, J. J. Xia, K. Jiang, Binyu Zhao, X. J. Hu, Yun-Feng Liang, W. Wang, Y. A. Han, J. G. Guo, Yu. V. Stenkin, Lang Shao, J.W. Xia, P. Pattarakijwanich, X. H. You, S.H. Chen, S. R. Zhang, C. Hou, Shuibin Lin, Lu Zhang, L. Feng, Xuelong Wang, S. Wu, X. X. Zhai, Xuliang Chen, C. X. Liu, L. L. Ma, Y. He, Z. X. Fan, Z. Y. You, F. R. Zhu, Y. W. Bao, Qie Sun, Yi Chen, X. G. Wang, Yi Zhang, Xiang-Yu Wang, D. H. Huang, R. Zhou, Hao Zhou, H. Zhu, X. J. Bi, D. della Volpe, Tao Zeng, T. L. Chen, Bin Ma, J. S. Wang, Cunguo Wang, L. X. Zhang, Shujuan Liu, N. Yin, N. Cheng, D. Bastieri, X. H. Cui, Cheng Li, W. J. Long, Shengxue Zhang, Axikegu, Li Zhang, G. H. Gong, Danzengluobu, M. H. Gu, Y. H. Yu, Jie Zhang, Y. Z. Fan, Dong Liu, C. Y. Wu, J. T. Cai, Long Chen, Y. Zheng, L. Q. Yin, Y. M. Ye, J. Y. Yang, B D Ettorre Piazzoli, David Ruffolo, Z. B. Sun, Cheng Guang Zhu, X. H. Ma, M. Heller, K. Li, Z. J. Jiang, J. Liu, Yong Zhang, Minghui Liu, R. N. Wang, and Jinyao Liu
Subjects: Physics, Multidisciplinary, Photon, COSMIC cancer database, Proton, Astrophysics::High Energy Astrophysical Phenomena, Astrophysics::Instrumentation and Methods for Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, Electron, Astrophysics, 01 natural sciences, Galaxy, Supernova, Crab Nebula, Pulsar, 0103 physical sciences, 010306 general physics, 010303 astronomy & astrophysics, Astrophysics::Galaxy Astrophysics
Abstract: The extension of the cosmic-ray spectrum beyond 1 petaelectronvolt (PeV; 1015 electronvolts) indicates the existence of the so-called PeVatrons—cosmic-ray factories that accelerate particles to PeV energies. We need to locate and identify such objects to find the origin of Galactic cosmic rays1. The principal signature of both electron and proton PeVatrons is ultrahigh-energy (exceeding 100 TeV) γ radiation. Evidence of the presence of a proton PeVatron has been found in the Galactic Centre, according to the detection of a hard-spectrum radiation extending to 0.04 PeV (ref. 2). Although γ-rays with energies slightly higher than 0.1 PeV have been reported from a few objects in the Galactic plane3–6, unbiased identification and in-depth exploration of PeVatrons requires detection of γ-rays with energies well above 0.1 PeV. Here we report the detection of more than 530 photons at energies above 100 teraelectronvolts and up to 1.4 PeV from 12 ultrahigh-energy γ-ray sources with a statistical significance greater than seven standard deviations. Despite having several potential counterparts in their proximity, including pulsar wind nebulae, supernova remnants and star-forming regions, the PeVatrons responsible for the ultrahigh-energy γ-rays have not yet been firmly localized and identified (except for the Crab Nebula), leaving open the origin of these extreme accelerators. Observations of γ-rays with energies up to 1.4 PeV find that 12 sources in the Galaxy are PeVatrons, one of which is the Crab Nebula.
Published: 2021

10. Prospect of detecting TeV halos with LHAASO: in the framework of the anisotropic diffusion model

Author: Kai Yan, Ruo-Yu Liu, S. Z. Chen, and Xiang-Yu Wang
Subjects: High Energy Astrophysical Phenomena (astro-ph.HE), Space and Planetary Science, Astrophysics::High Energy Astrophysical Phenomena, FOS: Physical sciences, Astronomy and Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, Astrophysics - High Energy Astrophysical Phenomena, Astrophysics::Galaxy Astrophysics
Abstract: The particle diffusion coefficients of three TeV pulsar halos observed so far are inferred to be significantly smaller than the typical value of the interstellar medium (ISM). The anisotropic diffusion model ascribes the slow diffusion to the cross-field diffusion assuming sub-Alfv{\'e}nic turbulence in the ISM around the pulsar if the viewing angle between the observer's line-of-sight (LOS) to the pulsar and the local mean field direction is small. In general, the TeV halo's morphology under this model highly depends on the viewing angle, and an elongated, asymmetric morphology is predicted if the LOS is not approximately aligned with the local mean field direction. While the specific requirement of a small viewing angle is supposedly established only for a small fraction of TeV halos, TeV halos with apparent asymmetric morphology has not been detected. In this paper we will study the expectation of TeV halos measured by the TeV-PeV gamma-ray detector LHAASO in the framework of anisotropic diffusion model, with a particular focus on the influence of the viewing angle on the detectability. We show that a TeV halo is more detectable with a smaller viewing angle and this selection effect may explain why the morphologies of all three detected TeV halos so far are consistent being spherical. We also demonstrate that LHAASO is capable of detecting asymmetric TeV halos after several-year operation with reasonable source parameters. This can serve as a critical test of the anisotropic diffusion model., Comment: 11 pages, 6 figure; submitted to ApJ
Published: 2022
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11. [The role of intestinal bacteria derived extracellular vesicles in inflammatory bowel disease]

Author: S Z, Chen and Y, Chen
Subjects: Extracellular Vesicles, Bacteria, Humans, Intestinal Mucosa, Colitis, Inflammatory Bowel Diseases
Abstract: 炎症性肠病（IBD）在我国发病率日益增长，因其诊断困难，无特异性治疗方法，预后差，依然有待深入研究。肠道菌群在各种肠内外疾病中发挥不可替代作用，而肠道细菌所分泌的细胞外囊泡与体细胞外泌体类似，在细胞间通讯、增殖、分化、炎症、恶变等过程中起重要作用。目前国内外关于细胞外囊泡在IBD的研究集中于人体细胞来源的细胞外囊泡，然而肠道细菌来源的细胞外囊泡同样在IBD中起着不可忽视的作用。本文就人体肠道菌群来源的细胞外囊泡在IBD发病中的作用机制进行综述，以期为IBD的诊断和治疗提供理论依据。.
Published: 2021

12. [Long-term therapeutic effects and liver fibrosis changes with direct-antiviral therapy in HIV/HCV co-infected patients]

Author: B L, Liao, L H, Li, H L, Zhong, H, Li, Y H, Li, S Z, Chen, C Y, Wen, F Y, Hu, Y, Lan, and W P, Cai
Subjects: Adult, Liver Cirrhosis, Male, Treatment Outcome, Coinfection, Humans, HIV Infections, Hepacivirus, Hepatitis C, Chronic, Antiviral Agents, Hepatitis C
Published: 2021

13. [Clinical characteristics and prognostic risk factors analysis of carbapenem-resistant organism in the department of hematology]

Author: S Z, Chen, J J, Xu, T T, Xiao, Y X, Weng, D B, Chen, Y, Zhang, J H, Ren, X F, Luo, Z H, Zheng, X Y, Zheng, Z Z, Chen, J D, Hu, and T, Yang
Subjects: 耐碳青霉烯类肠杆菌科细菌, Carbapenem-Resistant Organism, Hematology, Microbial Sensitivity Tests, Prognosis, Anti-Bacterial Agents, 论著, Carbapenem-Resistant Enterobacteriaceae, Carbapenems, Risk Factors, Humans, Risk factor, 碳青霉烯耐药革兰阴性杆菌, 危险因素, Retrospective Studies
Abstract: 目的了解血液科碳青霉烯耐药革兰阴性菌（CRO）感染的分布及耐药情况，分析影响CRO感染患者预后的危险因素，为临床CRO感染患者的治疗和预后判断提供依据。方法回顾性分析2018年1月至2020年6月血液科确诊的CRO感染患者181例，收集患者的临床和实验室检查等资料，分析影响患者30 d死亡的危险因素。在碳青霉烯类耐药肠杆菌科细菌（CRE）亚组中进一步评价CRE主动筛查的临床意义。结果分离出的181株CRO中CRE占47.2％，铜绿假单胞菌占37.0％，肺炎克雷伯菌占32.6％，对碳青霉烯类药物高度耐药，对亚胺培南耐药最低抑菌浓度（MIC）≥16 µg/ml的占76.8％（139/181）。菌株标本来源主要是血样和痰液。CRO和CRE感染患者30 d的全因死亡率分别为（41.4±3.7）％、（44.7±5.4）％。Cox多因素回归分析结果显示：降钙素原水平>0.2 ng/ml及亚胺培南耐药的MIC≥16 µg/ml是CRO感染30 d死亡的独立危险因素。CRE亚组分析结果显示，亚胺培南耐药的MIC≥16 µg/ml为CRE感染30 d死亡的独立危险因素。CRE主动筛查患者的30 d累积生存率高于未筛查患者［（68.0±9.3）％对（50.0±6.5）％，P＝0.21］。结论高亚胺培南耐药MIC值的致病菌严重影响血液科CRO感染患者预后，病死率高。开展CRE主动筛查有助于早期预防、早期诊断和早期治疗高危患者。
Published: 2021

14. Measurement of interplanetary magnetic field in short period using the cosmic-ray Sun shadow measured by LHAASO

Author: S. Z. Chen, Yuncheng Nan, and Cunfeng Feng
Subjects: Physics, Period (periodic table), Shadow, Astronomy, Cosmic ray, Interplanetary magnetic field
Published: 2021

15. The performances of the LHAASO-KM2A tested by the observation of cosmic-ray Moon shadow

Author: Zhe Li, Yizhuo Li, Yuncheng Nan, S. Z. Chen, Sha Wu, and Cunfeng Feng
Subjects: Physics, Shadow, Astronomy, Cosmic ray
Published: 2021

16. Discovery of a new $\gamma$-ray source LHAASO J0341+5258 with emission up to 200TeV

Author: Zhengguo Cao, L. Feng, Xufang Li, Zebo Tang, Jun-Jie Wei, C. Y. Wu, Jia Zhang, L. X. Bai, Yi Zhang, H. K. Lv, Jixia Li, L. L. Yang, Z. X. Wang, M. Zha, Y. M. Ye, X. H. Ma, L. P. Wang, X. G. Wang, Donglian Xu, X. L. Guo, Y. A. Han, Binyu Zhao, Yun-Feng Liang, Houdun Zeng, Zhe Li, Y. Su, B. Z. Dai, Z. G. Dai, Jinmei Liu, B. D'Ettorre Piazzoli, Z. G. Yao, Y. Zheng, W. X. Wu, M. L. Chen, Jianeng Zhou, Hefan Li, W. Wang, P. Pattarakijwanich, Rong Xu, J. J. Xia, X. X. Zhai, J. Fang, F. R. Zhu, Qie Sun, Yi Chen, H. B. Li, G. M. Xiang, W. Liu, B. Y. Pang, S. Wu, X. L. Ji, R. Lu, K. Li, Y. J. Bi, H. D. Liu, Y. D. Cheng, Bo Zhang, L. Q. Yin, Hanzhong Zhang, C. X. Liu, D. della Volpe, Y. D. Cui, Kun Fang, Yugang Zhang, E. W. Liang, Ping Zhou, Z. J. Jiang, Y. J. Wei, J. Liu, Yong Zhang, Duo Yan, Yu. V. Stenkin, S. L. He, Y. P. Wang, Z. X. Liu, D. H. Huang, R. N. Wang, S. M. Liu, F. Ji, V. Rulev, Y. Z. Li, H. H. He, H. Zhu, C. Hou, Zheng Wang, B. Q. Ma, Y. C. Nan, L. Xue, Jun Liu, Lu Zhang, H. Y. Jia, D. M. Wei, V. I. Stepanov, E. S. Chen, Sina Chen, K. J. Zhu, Y. Q. Qi, Fulai Guo, J. Y. Shi, Minghui Liu, Yi Liu, J. B. Zhao, H. Wang, X. F. Wu, Zhen Wang, Z. X. Fan, Z. Y. You, Shi-Qi Hu, J. Y. Yang, N. Cheng, Z. K. Zeng, C. D. Gao, X. H. You, Long Gao, H. C. Song, Lei Zhao, D.A. Kuleshov, X. X. Zhou, Q. Yuan, B. M. Chen, Ruizhi Yang, X. N. Sun, Shengxue Zhang, Danzengluobu, J. F. Chang, S. P. Zhao, H. Liu, J.W. Xia, W. Gao, G. C. Xiao, Felix Aharonian, Xinbo He, K. Jiang, Pak-Hin Thomas Tam, H. C. Li, Y. Wang, Y. Z. Fan, Dong Liu, Y. W. Bao, P. F. Zhang, X. J. Bi, H. N. He, T. L. Chen, L. Z. Zhao, X. J. Hu, R. Zhou, Ying Zhang, Oleg Shchegolev, Junjie Mao, Y. Q. Guo, F. Y. Li, K. Levochkin, J. T. Cai, X. D. Sheng, Cong Li, X. Zuo, B. B. Li, Long Chen, Yunchao Liu, H. L. Dai, T. Wen, S. W. Cui, S. Z. Chen, David Ruffolo, Y. M. Xing, H. R. Wu, Liang Chen, Xiang-Kun Dong, S. Hu, J. Y. Liu, X. Y. Huang, P. P. Zhang, X. H. Cui, Minghao Qi, Z. B. Sun, Y. Bai, Z. Y. Pei, Cheng Guang Zhu, Yuan-Hao Wang, Zhuo Li, Warit Mitthumsiri, H. M. Zhang, Q. An, Y. H. Yao, W. H. Huang, H. Zhou, W. J. Long, Binbin Zhou, Li-Sheng Geng, R. Liu, Xiang Zhang, J. G. Guo, J. W. Zhang, S. R. Zhang, Wenwu Tian, L. L. Ma, Q. Gao, C. F. Feng, Jiangang He, J. S. Wang, Cunguo Wang, Y. L. Xin, Z. C. Huang, H. B. Hu, N. Yin, B. Q. Qiao, Xin Li, Cheng Li, Jiajun Qin, M. H. Gu, Boyang Wang, Rui Zhang, H. B. Xiao, W. Zeng, L. X. Zhang, S. H. Feng, M. M. Ge, Axikegu, Yonggang Wang, M. J. Chen, Zhao-Qi Wang, Y. Y. Guo, Li Zhang, G. H. Gong, Zhe Cao, Y. K. Hor, Y. H. Yu, T. Montaruli, Jian Wang, Chiming Jin, Z. Min, Xuelong Wang, G. G. Xin, Kai-Kai Duan, D. Bastieri, Y. L. Feng, T. Ke, S. J. Lin, X. T. Huang, L. Y. Wang, B. Liu, Jingzhi Yan, Bingshui Gao, Xiang-Yu Wang, Yulong Li, Tao Zeng, Xuliang Chen, Y. He, C. W. Yang, Jun-Hui Fan, Q. B. Gou, W. L. Li, D. X. Xiao, Qizhi Huang, J. Chen, Xiao-Hu Zhang, H. Cai, M. J. Yang, S. Q. Xi, Hong-Guang Wang, Alejandro Sáiz, Q. H. Chen, S. B. Yang, Fan Yang, A. Masood, F. Zheng, Lang Shao, and M. Heller
Subjects: Physics, Astrophysics::High Energy Astrophysical Phenomena, Hadron, Gamma ray, Flux, Astronomy and Astrophysics, Astrophysics, Galactic plane, Crab Nebula, Pulsar, Space and Planetary Science, Angular diameter, High Energy Physics::Experiment, Supernova remnant, Astrophysics - High Energy Astrophysical Phenomena, Astrophysics::Galaxy Astrophysics
Abstract: We report the discovery of a new unidentified extended $\gamma$-ray source in the Galactic plane named LHAASO J0341+5258 with a pre-trial significance of 8.2 standard deviations above 25 TeV. The best fit position is R.A.$=55.34^{\circ}\pm0.11^{\circ}$ and Dec$=52.97^{\circ}\pm0.07^{\circ}$. The angular size of LHAASO J0341+5258 is $0.29^\circ \pm 0.06^\circ_{stat} \pm0.02^\circ_{sys}$. The flux above 25 TeV is about $20\%$ of the flux of Crab Nebula. Although a power-law fit of the spectrum from 10 TeV to 200 TeV with the photon index $\alpha=2.98 \pm 0.19_{stat} \pm 0.02_{sys}$ is not excluded, the LHAASO data together with the flux upper limit at 10 GeV set by the Fermi LAT observation, indicate a noticeable steepening of an initially hard power-law spectrum %($\alpha \leq 1.75$) spectrum with a cutoff at $\approx 50$ TeV. We briefly discuss the origin of UHE gamma-rays. The lack of an energetic pulsar and a young SNR inside or in the vicinity of LHAASO J0341+5258 challenge, but do not exclude both the leptonic and hadronic scenarios of gamma-ray production., Comment: Accepted by APJL
Published: 2021

17. Simulation Study on Scaler Mode in LHAASO-KM2A

Author: Jing Zhao, Xunxiu Zhou, Zhicheng Huang, Bing Zhao, Daihui Huang, Kegu Axi, Dong Liu, S. Z. Chen, Huihai He, and Xinhua Ma
Subjects: Nuclear physics, Physics, Detector, Mode (statistics), Cosmic ray, Independent data, Event (particle physics), Coincidence, Energy (signal processing), Muon detector
Abstract: LHAASO, located at Daocheng in Sichuan province of China with an altitude up to 4410 m above the sea level, takes the function of hybrid technology to detect cosmic rays. As the major array of LHAASO, KM2A is composed of 5195 electromagnetic particle detectors (EDs) and 1188 muon detectors (MDs). In the ground-based experiments, there are two common independent data acquisition systems, corresponding to the scaler and shower operation modes. In order to learn more about the scaler mode in LHAASO-KM2A, we adopt the CORSIKA to study the shower development and employ the G4KM2A (based on Geant4) to simulate the detector responses. For one cluster (composed of 64 EDs) in the array of KM2A-ED, the event rates of showers having a number of fired EDs ≥ 1, 2, 3 and 4 (in a time coincidence of 100 ns) are recorded. The average rates of the four multiplicities are ∼ 88 kHz, ∼ 1.4 kHz, ∼ 210 Hz and ∼110 Hz, respectively. For the array of KM2A-MD, there are 16 MDs in one cluster. The average rates with multiplicities ≥ 1 and 2 are ∼ 84 kHz and ∼ 890 Hz, respectively. The corresponding primary energies are also given. According to our simulations, the energy threshold of the scaler mode can be lowered to ∼ 100 GeV. At the same time, the energy threshold of LHAASO-KM2A in shower mode is presented for comparison. The simulation results in this work are beneficial for the online trigger with scaler mode, and also be useful in understanding the experiment results in LHAASO-KM2A.
Published: 2021

18. Exploring Lorentz Invariance Violation from Ultrahigh-Energy γ Rays Observed by LHAASO

Author: Zhen, Cao, F, Aharonian, Q, An, Axikegu, L X, Bai, Y X, Bai, Y W, Bao, D, Bastieri, X J, Bi, Y J, Bi, H, Cai, J T, Cai, Zhe, Cao, J, Chang, J F, Chang, B M, Chen, E S, Chen, J, Chen, Liang, Chen, Long, Chen, M J, Chen, M L, Chen, Q H, Chen, S H, Chen, S Z, Chen, T L, Chen, X L, Chen, Y, Chen, N, Cheng, Y D, Cheng, S W, Cui, X H, Cui, Y D, Cui, B D'Ettorre, Piazzoli, B Z, Dai, H L, Dai, Z G, Dai, Danzengluobu, D, Della Volpe, X J, Dong, K K, Duan, J H, Fan, Y Z, Fan, Z X, Fan, J, Fang, K, Fang, C F, Feng, L, Feng, S H, Feng, Y L, Feng, B, Gao, C D, Gao, L Q, Gao, Q, Gao, W, Gao, M M, Ge, L S, Geng, G H, Gong, Q B, Gou, M H, Gu, F L, Guo, J G, Guo, X L, Guo, Y Q, Guo, Y Y, Guo, Y A, Han, H H, He, H N, He, J C, He, S L, He, X B, He, Y, He, M, Heller, Y K, Hor, C, Hou, X, Hou, H B, Hu, S, Hu, S C, Hu, X J, Hu, D H, Huang, Q L, Huang, W H, Huang, X T, Huang, X Y, Huang, Z C, Huang, F, Ji, X L, Ji, H Y, Jia, K, Jiang, Z J, Jiang, C, Jin, T, Ke, D, Kuleshov, K, Levochkin, B B, Li, Cheng, Li, Cong, Li, F, Li, H B, Li, H C, Li, H Y, Li, Jian, Li, Jie, Li, K, Li, W L, Li, X R, Li, Xin, Li, Y, Li, Y Z, Li, Zhe, Li, Zhuo, Li, E W, Liang, Y F, Liang, S J, Lin, B, Liu, C, Liu, D, Liu, H, Liu, H D, Liu, J, Liu, J L, Liu, J S, Liu, J Y, Liu, M Y, Liu, R Y, Liu, S M, Liu, W, Liu, Y, Liu, Y N, Liu, Z X, Liu, W J, Long, R, Lu, H K, Lv, B Q, Ma, L L, Ma, X H, Ma, J R, Mao, A, Masood, Z, Min, W, Mitthumsiri, T, Montaruli, Y C, Nan, B Y, Pang, P, Pattarakijwanich, Z Y, Pei, M Y, Qi, Y Q, Qi, B Q, Qiao, J J, Qin, D, Ruffolo, V, Rulev, A, Sáiz, L, Shao, O, Shchegolev, X D, Sheng, J R, Shi, H C, Song, Yu V, Stenkin, V, Stepanov, Y, Su, Q N, Sun, X N, Sun, Z B, Sun, P H T, Tam, Z B, Tang, W W, Tian, B D, Wang, C, Wang, H, Wang, H G, Wang, J C, Wang, J S, Wang, L P, Wang, L Y, Wang, R N, Wang, W, Wang, X G, Wang, X J, Wang, X Y, Wang, Y, Wang, Y D, Wang, Y J, Wang, Y P, Wang, Z H, Wang, Z X, Wang, Zhen, Wang, Zheng, Wang, D M, Wei, J J, Wei, Y J, Wei, T, Wen, C Y, Wu, H R, Wu, S, Wu, W X, Wu, X F, Wu, S Q, Xi, J, Xia, J J, Xia, G M, Xiang, D X, Xiao, G, Xiao, H B, Xiao, G G, Xin, Y L, Xin, Y, Xing, D L, Xu, R X, Xu, L, Xue, D H, Yan, J Z, Yan, C W, Yang, F F, Yang, J Y, Yang, L L, Yang, M J, Yang, R Z, Yang, S B, Yang, Y H, Yao, Z G, Yao, Y M, Ye, L Q, Yin, N, Yin, X H, You, Z Y, You, Y H, Yu, Q, Yuan, H D, Zeng, T X, Zeng, W, Zeng, Z K, Zeng, M, Zha, X X, Zhai, B B, Zhang, H M, Zhang, H Y, Zhang, J L, Zhang, J W, Zhang, L X, Zhang, Li, Zhang, Lu, Zhang, P F, Zhang, P P, Zhang, R, Zhang, S R, Zhang, S S, Zhang, X, Zhang, X P, Zhang, Y F, Zhang, Y L, Zhang, Yi, Zhang, Yong, Zhang, B, Zhao, J, Zhao, L, Zhao, L Z, Zhao, S P, Zhao, F, Zheng, Y, Zheng, B, Zhou, H, Zhou, J N, Zhou, P, Zhou, R, Zhou, X X, Zhou, C G, Zhu, F R, Zhu, H, Zhu, K J, Zhu, and X, Zuo
Subjects: General Physics and Astronomy
Abstract: Recently, the LHAASO Collaboration published the detection of 12 ultrahigh-energy γ-ray sources above 100 TeV, with the highest energy photon reaching 1.4 PeV. The first detection of PeV γ rays from astrophysical sources may provide a very sensitive probe of the effect of the Lorentz invariance violation (LIV), which results in decay of high-energy γ rays in the superluminal scenario and hence a sharp cutoff of the energy spectrum. Two highest energy sources are studied in this work. No signature of the existence of the LIV is found in their energy spectra, and the lower limits on the LIV energy scale are derived. Our results show that the first-order LIV energy scale should be higher than about 10^{5} times the Planck scale M_{Pl} and that the second-order LIV scale is10^{-3}M_{Pl}. Both limits improve by at least one order of magnitude the previous results.
Published: 2021

19. Study of the trigger mode of LHAASO-KM2A

Author: Liang Chen, Yuncheng Nan, Hongkui Lv, Jia Liu, Wei Gao, S. Z. Chen, Cong Li, Ye Liu, Sha Wu, Huihai He, and Zhe Li
Subjects: Physics, 010308 nuclear & particles physics, business.industry, Astrophysics::High Energy Astrophysical Phenomena, Detector, Astronomy and Astrophysics, Cosmic ray, Threshold energy, 01 natural sciences, Coincidence, Air shower, Software, Optics, Observatory, 0103 physical sciences, business, 010303 astronomy & astrophysics, Noise (radio)
Abstract: The Large High Altitude Air Shower Observatory (LHAASO), built 4410 m a.s.l. near Daocheng, in the Sichuan province of China, is a new-generation complex EAS array. The Square Kilometre Array (KM2A), one of LHAASO’s three detector arrays, is composed of 5195 electromagnetic particle detectors and 1171 muon detectors, which are distributed in an area of 1.3 km2. A lower trigger threshold would increase the number of low-energy showers detected, although this would also import many noise events because of the numerous KM2A detectors. In this work, the KM2A trigger logic adopted a software trigger system. A toy simulation was developed to estimate the chance coincidence rate of noise hits. Taking into account the characteristics of real cosmic ray shower events, the trigger logic was investigated by adjusting the space and time windows simultaneously using the detector simulation sample. In order to improve trigger efficiency and reduce the effect of noise, an optimized trigger criterion was achieved. The KM2A threshold energy can be reduced to 5 TeV. The performance of KM2A with this trigger criterion is presented. The expectation on observation of sun shadow and cosmic ray large-scale anisotropy are also shown.
Published: 2018

20. Extended Very-High-Energy Gamma-Ray Emission Surrounding PSR J0622+3749 Observed by LHAASO-KM2A

Author: F, Aharonian, Q, An, Axikegu, L X, Bai, Y X, Bai, Y W, Bao, D, Bastieri, X J, Bi, Y J, Bi, H, Cai, J T, Cai, Z, Cao, J, Chang, J F, Chang, X C, Chang, B M, Chen, J, Chen, L, Chen, M J, Chen, M L, Chen, Q H, Chen, S H, Chen, S Z, Chen, T L, Chen, X L, Chen, Y, Chen, N, Cheng, Y D, Cheng, S W, Cui, X H, Cui, Y D, Cui, B Z, Dai, H L, Dai, Z G, Dai, Danzengluobu, D, Della Volpe, B, D'Ettorre Piazzoli, X J, Dong, J H, Fan, Y Z, Fan, Z X, Fan, J, Fang, K, Fang, C F, Feng, L, Feng, S H, Feng, Y L, Feng, B, Gao, C D, Gao, Q, Gao, W, Gao, M M, Ge, L S, Geng, G H, Gong, Q B, Gou, M H, Gu, J G, Guo, X L, Guo, Y Q, Guo, Y Y, Guo, Y A, Han, H H, He, H N, He, J C, He, S L, He, X B, He, Y, He, M, Heller, Y K, Hor, C, Hou, X, Hou, H B, Hu, S, Hu, S C, Hu, X J, Hu, D H, Huang, Q L, Huang, W H, Huang, X T, Huang, Z C, Huang, F, Ji, X L, Ji, H Y, Jia, K, Jiang, Z J, Jiang, C, Jin, D, Kuleshov, K, Levochkin, B B, Li, C, Li, F, Li, H B, Li, H C, Li, H Y, Li, J, Li, K, Li, W L, Li, X, Li, X R, Li, Y, Li, Y Z, Li, Z, Li, E W, Liang, Y F, Liang, S J, Lin, B, Liu, C, Liu, D, Liu, H, Liu, H D, Liu, J, Liu, J L, Liu, J S, Liu, J Y, Liu, M Y, Liu, R Y, Liu, S M, Liu, W, Liu, Y N, Liu, Z X, Liu, W J, Long, R, Lu, H K, Lv, B Q, Ma, L L, Ma, X H, Ma, J R, Mao, A, Masood, W, Mitthumsiri, T, Montaruli, Y C, Nan, B Y, Pang, P, Pattarakijwanich, Z Y, Pei, M Y, Qi, D, Ruffolo, V, Rulev, A, Sáiz, L, Shao, O, Shchegolev, X D, Sheng, J R, Shi, H C, Song, Yu V, Stenkin, V, Stepanov, Q N, Sun, X N, Sun, Z B, Sun, P H T, Tam, Z B, Tang, W W, Tian, B D, Wang, C, Wang, H, Wang, H G, Wang, J C, Wang, J S, Wang, L P, Wang, L Y, Wang, R N, Wang, W, Wang, X G, Wang, X J, Wang, X Y, Wang, Y D, Wang, Y J, Wang, Y P, Wang, Z, Wang, Z H, Wang, Z X, Wang, D M, Wei, J J, Wei, Y J, Wei, T, Wen, C Y, Wu, H R, Wu, S, Wu, W X, Wu, X F, Wu, S Q, Xi, J, Xia, J J, Xia, G M, Xiang, G, Xiao, H B, Xiao, G G, Xin, Y L, Xin, Y, Xing, D L, Xu, R X, Xu, L, Xue, D H, Yan, C W, Yang, F F, Yang, J Y, Yang, L L, Yang, M J, Yang, R Z, Yang, S B, Yang, Y H, Yao, Z G, Yao, Y M, Ye, L Q, Yin, N, Yin, X H, You, Z Y, You, Y H, Yu, Q, Yuan, H D, Zeng, T X, Zeng, W, Zeng, Z K, Zeng, M, Zha, X X, Zhai, B B, Zhang, H M, Zhang, H Y, Zhang, J L, Zhang, J W, Zhang, L, Zhang, L X, Zhang, P F, Zhang, P P, Zhang, R, Zhang, S R, Zhang, S S, Zhang, X, Zhang, X P, Zhang, Y, Zhang, Y F, Zhang, Y L, Zhang, B, Zhao, J, Zhao, L, Zhao, L Z, Zhao, S P, Zhao, F, Zheng, Y, Zheng, B, Zhou, H, Zhou, J N, Zhou, P, Zhou, R, Zhou, X X, Zhou, C G, Zhu, F R, Zhu, H, Zhu, K J, Zhu, X, Zuo, and X Y, Huang
Abstract: We report the discovery of an extended very-high-energy (VHE) gamma-ray source around the location of the middle-aged (207.8 kyr) pulsar PSR J0622+3749 with the Large High-Altitude Air Shower Observatory (LHAASO). The source is detected with a significance of 8.2σ for E25 TeV assuming a Gaussian template. The best-fit location is (right ascension, declination) =(95.47°±0.11°,37.92°±0.09°), and the extension is 0.40°±0.07°. The energy spectrum can be described by a power-law spectrum with an index of -2.92±0.17_{stat}±0.02_{sys}. No clear extended multiwavelength counterpart of the LHAASO source has been found from the radio to sub-TeV bands. The LHAASO observations are consistent with the scenario that VHE electrons escaped from the pulsar, diffused in the interstellar medium, and scattered the interstellar radiation field. If interpreted as the pulsar halo scenario, the diffusion coefficient, inferred for electrons with median energies of ∼160 TeV, is consistent with those obtained from the extended halos around Geminga and Monogem and much smaller than that derived from cosmic ray secondaries. The LHAASO discovery of this source thus likely enriches the class of so-called pulsar halos and confirms that high-energy particles generally diffuse very slowly in the disturbed medium around pulsars.
Published: 2021

21. [Changes and clinical significance of serum NSE and MBP levels in children with cerebral palsy at high altitude during comprehensive rehabilitation]

Author: S Z, Chen, J L, Liu, X R, A, P L, Ren, and Y, Yang
Subjects: Male, Diagnostic Tests, Routine, Altitude, Cerebral Palsy, Child, Preschool, Phosphopyruvate Hydratase, Humans, Female, Myelin Basic Protein, Child
Published: 2021

22. Discovery of the Ultra-high energy gamma-ray source LHAASO J2108+5157

Author: Zhen Cao, F. Aharonian, Q. An, null Axikegu, L. X. Bai, Y. X. Bai, Y. W. Bao, D. Bastieri, X. J. Bi, Y. J. Bi, H. Cai, J. T. Cai, Zhe Cao, J. Chang, J. F. Chang, B. M. Chen, E. S. Chen, J. Chen, Liang Chen, Long Chen, M. J. Chen, M. L. Chen, Q. H. Chen, S. H. Chen, S. Z. Chen, T. L. Chen, X. L. Chen, Y. Chen, N. Cheng, Y. D. Cheng, S. W. Cui, X. H. Cui, Y. D. Cui, B. D’Ettorre Piazzoli, B. Z. Dai, H. L. Dai, Z. G. Dai, Dan-Zeng Dan-Zeng-Luo-Bu, D. della Volpe, X. J. Dong, K. K. Duan, J. H. Fan, Y. Z. Fan, Z. X. Fan, J. Fang, K. Fang, C. F. Feng, L. Feng, S. H. Feng, Y. L. Feng, B. Gao, C. D. Gao, L. Q. Gao, Q. Gao, W. Gao, M. M. Ge, L. S. Geng, G. H. Gong, Q. B. Gou, M. H. Gu, F. L. Guo, J. G. Guo, X. L. Guo, Y. Q. Guo, Y. Y. Guo, Y. A. Han, H. H. He, H. N. He, J. C. He, S. L. He, X. B. He, Y. He, M. Heller, Y. K. Hor, C. Hou, H. B. Hu, S. Hu, S. C. Hu, X. J. Hu, D. H. Huang, Q. L. Huang, W. H. Huang, X. T. Huang, X. Y. Huang, Z. C. Huang, F. Ji, X. L. Ji, H. Y. Jia, K. Jiang, Z. J. Jiang, C. Jin, T. Ke, D. Kuleshov, K. Levochkin, B. B. Li, Cheng Li, Cong Li, F. Li, H. B. Li, H. C. Li, H. Y. Li, J. Li, K. Li, W. L. Li, X. R. Li, Xin Li, Y. Li, Y. Z. Li, Zhe Li, Zhuo Li, E. W. Liang, Y. F. Liang, S. J. Lin, B. Liu, C. Liu, D. Liu, H. Liu, H. D. Liu, J. Liu, J. L. Liu, J. S. Liu, J. Y. Liu, M. Y. Liu, R. Y. Liu, S. M. Liu, W. Liu, Y. Liu, Y. N. Liu, Z. X. Liu, W. J. Long, R. Lu, H. K. Lv, B. Q. Ma, L. L. Ma, X. H. Ma, J. R. Mao, A. Masood, Z. Min, W. Mitthumsiri, T. Montaruli, Y. C. Nan, B. Y. Pang, P. Pattarakijwanich, Z. Y. Pei, M. Y. Qi, Y. Q. Qi, B. Q. Qiao, J. J. Qin, D. Ruffolo, V. Rulev, A. Sáiz, L. Shao, O. Shchegolev, X. D. Sheng, J. Y. Shi, H. C. Song, Yu. V. Stenkin, V. Stepanov, Y. Su, Q. N. Sun, X. N. Sun, Z. B. Sun, P. H. T. Tam, Z. B. Tang, W. W. Tian, B. D. Wang, C. Wang, H. Wang, H. G. Wang, J. C. Wang, J. S. Wang, L. P. Wang, L. Y. Wang, R. N. Wang, W. Wang, X. G. Wang, X. J. Wang, X. Y. Wang, Y. Wang, Y. D. Wang, Y. J. Wang, Y. P. Wang, Z. H. Wang, Z. X. Wang, Zhen Wang, Zheng Wang, D. M. Wei, J. J. Wei, Y. J. Wei, T. Wen, C. Y. Wu, H. R. Wu, S. Wu, W. X. Wu, X. F. Wu, S. Q. Xi, J. Xia, J. J. Xia, G. M. Xiang, D. X. Xiao, G. Xiao, H. B. Xiao, G. G. Xin, Y. L. Xin, Y. Xing, D. L. Xu, R. X. Xu, L. Xue, D. H. Yan, J. Z. Yan, C. W. Yang, F. F. Yang, J. Y. Yang, L. L. Yang, M. J. Yang, R. Z. Yang, S. B. Yang, Y. H. Yao, Z. G. Yao, Y. M. Ye, L. Q. Yin, N. Yin, X. H. You, Z. Y. You, Y. H. Yu, Q. Yuan, H. D. Zeng, T. X. Zeng, W. Zeng, Z. K. Zeng, M. Zha, X. X. Zhai, B. B. Zhang, H. M. Zhang, H. Y. Zhang, J. L. Zhang, J. W. Zhang, L. X. Zhang, Li Zhang, Lu Zhang, P. F. Zhang, P. P. Zhang, R. Zhang, S. R. Zhang, S. S. Zhang, X. Zhang, X. P. Zhang, Y. F. Zhang, Y. L. Zhang, Yi Zhang, Yong Zhang, B. Zhao, J. Zhao, L. Zhao, L. Z. Zhao, S. P. Zhao, F. Zheng, Y. Zheng, B. Zhou, H. Zhou, J. N. Zhou, P. Zhou, R. Zhou, X. X. Zhou, C. G. Zhu, F. R. Zhu, H. Zhu, K. J. Zhu, and X. Zuo
Subjects: Physics, High Energy Astrophysical Phenomena (astro-ph.HE), Molecular cloud, Astrophysics::High Energy Astrophysical Phenomena, Hadron, Gamma ray, Flux, Sigma, FOS: Physical sciences, Astronomy and Astrophysics, Astrophysics, Gamma-ray astronomy, Space and Planetary Science, Energy spectrum, Ultrahigh energy, Astrophysics - High Energy Astrophysical Phenomena
Abstract: We report the discovery of a UHE gamma-ray source, LHAASO J2108+5157, by analyzing the LHAASO-KM2A data of 308.33 live days. Significant excess of gamma-ray induced showers is observed in both energy bands of 25-100 TeV and $\gt$100 TeV with 9.5 sigma and 8.5 sigma, respectively. This source is not significantly favored as an extensive source with the angular extension smaller than the point-spread function of KM2A. The measured energy spectrum from 20 to 200 TeV can be approximately described by a power-law function with an index of -2.83$\pm$ 0.18stat. A harder spectrum is demanded at lower energies considering the flux upper limit set by Fermi-LAT observations. The position of the gamma-ray emission is correlated with a giant molecular cloud, which favors a hadronic origin. No obvious counterparts have been found, deeper multiwavelength observations will help to shed new light on this intriguing UHE source., Comment: 12 pages, 7 figures, accepted by ApJL
Published: 2021
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23. Clinical epidemiology and outcome of HIV-associated talaromycosis in Guangdong, China, during 2011–2017

Author: M Chen, X Ou, P L Guo, S Z Chen, S G Wang, Weiping Cai, C Y Wen, Y R Li, W S Chen, Y Cao, Thuy Le, Yan Guo, Liya Li, R S Ying, Xiaoping Tang, and C B Luo
Subjects: 0301 basic medicine, Adult, Male, medicine.medical_specialty, China, HIV Infections, Disease, Article, 03 medical and health sciences, chemistry.chemical_compound, Penicilliosis, Young Adult, 0302 clinical medicine, Weight loss, Internal medicine, Epidemiology, medicine, Prevalence, Humans, Pharmacology (medical), 030212 general & internal medicine, Aged, Retrospective Studies, Creatinine, business.industry, Health Policy, Incidence (epidemiology), Incidence, Middle Aged, medicine.disease, Prognosis, 030112 virology, Elevated alkaline phosphatase, Hospitalization, Infectious Diseases, Logistic Models, chemistry, Mycoses, Histopathology, Female, Seasons, medicine.symptom, business
Abstract: Objectives Talaromycosis is an invasive mycosis endemic to Southeast Asia. This study aimed to investigate the epidemiology, clinical features and prognostic factors of HIV-associated talaromycosis in Guangdong, China. Methods We retrospectively evaluated HIV patients hospitalized with histopathology- or culture-confirmed talaromycosis between 2011 and 2017. Factors associated with poor prognosis were identified using logistic regression. Results Overall, 1079 patients with HIV-associated talaromycosis were evaluated. Both the number and prevalence of talaromycosis among HIV admissions increased from 125 and 15.7% in 2011 to 253 and 18.8% in 2017, respectively, reflecting the increase in HIV admissions. Annual admissions peaked during the rainy season between March and August. Common clinical manifestations included fever (85.6%), peripheral lymphadenopathy (72.3%), respiratory symptoms (60.8%), weight loss (49.8%), skin lesions (44.5%) and gastrointestinal symptoms (44.3%). Common laboratory abnormalities were hypoalbuminaemia (98.6%), anaemia (95.6%), elevated aspartate aminotransferase level (AST) (76.9%), elevated alkaline phosphatase level (55.8%) and thrombocytopenia (53.7%). The median CD4 count was 9 cells/μL. Talaromyces marneffei was isolated from blood and bone marrow cultures of 66.6% and 74.5% of patients, respectively. The rate increased to 86.6% when both cultures were performed concurrently. At discharge, 14% of patients showed worsening conditions or died. Leucocytosis, thrombocytopenia, elevated AST, total bilirubin, creatinine and azole monotherapy independently predicted poor prognosis. Conclusions The incidence of HIV-associated talaromycosis has increased in Guangdong with the high HIV burden in China. Skin lesions were seen in less than half of patients. Induction therapy with azole alone is associated with higher mortality. Findings from this study should help to improve treatment of the disease.
Published: 2020

24. Morphology of Gamma-Ray Halos around Middle-Aged Pulsars: Influence of the Pulsar Proper Motion

Author: Ruo-Yu Liu, S. Z. Chen, Xiang-Yu Wang, and Yi Zhang
Subjects: High Energy Astrophysical Phenomena (astro-ph.HE), Physics, Proper motion, Astrophysics::High Energy Astrophysical Phenomena, Astrophysics::Instrumentation and Methods for Astrophysics, FOS: Physical sciences, Astronomy and Astrophysics, Observable, Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, Pulsar, Space and Planetary Science, Halo, Surface brightness, Disc, Astrophysics - High Energy Astrophysical Phenomena, Proper velocity, Cherenkov radiation, Astrophysics::Galaxy Astrophysics
Abstract: Recently, gamma-ray halos of a few degree extension have been detected around two middle-aged pulsars, namely, Geminga and PSR B0656+14, by the High Altitude Water Cherenkov observatory (HAWC). The gamma-ray radiation arise from relativistic electrons that escape the pulsar wind nebula and diffuse in the surrounding medium. The diffusion coefficient is found to be significantly lower than the average value in the Galactic disk. If so, given a typical transverse velocity of $300-500{\,\rm km /s}$ for a pulsar, its displacement could be important in shaping the morphology of its gamma-ray halos. Motivated by this, we study the morphology of pulsar halos considering the proper motion of pulsar. We define three evolutionary phases of pulsar halo to categorize its morphological features. The morphology of pulsar halos below 10$\,$TeV is double peaked or single peaked with an extended tail, which depends on the electron injection history. Above 10 TeV, the morphology of pulsar halos is nearly spherical, due to the short cooling timescale ($, 20 pages, 14 figures, 3 tables, accepted by APJ
Published: 2020

25. Absolute calibration of LHAASO WFCTA camera based on LED

Author: W. J. Long, Rong Xu, Cong Li, J. J. Xia, Houdun Zeng, Axikegu, Yongchun Wang, H. H. He, Xufang Li, X. X. Zhai, Y. D. Cui, L. Feng, H. B. Li, F. R. Zhu, Qie Sun, Yi Chen, F. Y. Li, C. F. Feng, D. H. Huang, Bin Zhou, J. Y. Shi, V. I. Stepanov, H. Zhu, Jun-Jie Wei, L. Z. Zhao, F. Ji, M. Zha, Jia Zhang, Y. H. Yao, Yi Zhang, B. Q. Qiao, Rui Zhang, Linbin Yang, Zhengguo Cao, M. L. Chen, Jianeng Zhou, Jian Wang, Chiming Jin, Zhe Cao, M. M. Ge, X. Zuo, Xuliang Chen, D.A. Kuleshov, Hong-Guang Wang, Y. He, Xiang-Yu Wang, E. S. Chen, Y. A. Han, N. Cheng, J. Fang, S. Hu, J. Y. Liu, G. M. Xiang, H. C. Song, S. P. Zhao, Zebo Tang, H. B. Xiao, W. Liu, L. X. Bai, Binyu Zhao, Yun-Feng Liang, Tao Zeng, Jixia Li, W. Zeng, Bin Ma, Donglian Xu, Z. Min, Xuelong Wang, Xiaofei Zhang, X. L. Guo, X. J. Dong, Hefan Li, S. H. Feng, Q. H. Chen, G. G. Xin, Warit Mitthumsiri, Kai-Kai Duan, Ying Zhang, P. F. Zhang, Z. X. Wang, H.Y. Gan, T. Wen, S. W. Cui, K. Levochkin, Hao Zhou, W. Wang, P. Pattarakijwanich, Kun Fang, D. M. Wei, H. Cai, S. Wu, Sina Chen, X. D. Sheng, Minghao Qi, C. X. Liu, Y. L. Feng, D. Bastieri, Q. An, B. Y. Pang, B. Liu, B. D. Wang, T. Ke, S. B. Yang, Bai Yibing, Lidan Gao, Y. W. Bao, Y. C. Nan, S. Z. Chen, Zhe Li, Shi-Qi Hu, X. H. You, H. B. Hu, H. Liu, X. T. Huang, J. C. He, Bingshui Gao, R. Zhou, L. Y. Wang, Z. H. Wang, Li Zhang, Z. G. Dai, M. J. Yang, Fan Yang, A. Masood, David Ruffolo, C. W. Yang, Q. Gao, Jun Liu, Z. K. Zeng, C. D. Gao, Lei Zhao, Z. C. Huang, B. B. Li, G. H. Gong, Lang Shao, M. J. Chen, Y. J. Wang, H. M. Zhang, D. della Volpe, He Zhang, Jianguo Qin, Y. J. Bi, Jun-Hui Fan, H. D. Liu, W. H. Huang, Y. D. Cheng, Z. B. Sun, Bo Zhang, Duo Yan, Z. X. Liu, Ruizhi Yang, X. N. Sun, Li-Sheng Geng, S. L. He, W. L. Li, Y. P. Wang, Y. H. Yu, Z. G. Yao, D. X. Xiao, J.W. Xia, X. G. Wang, H. L. Dai, Y. Y. Guo, Danzengluobu, Y. Q. Qi, H. Wang, W. Gao, Yi Liu, J. B. Zhao, Y. K. Hor, J. Chen, Zheng Wang, Q. B. Gou, L. P. Wang, Qizhi Huang, T. L. Chen, X. F. Wu, X. L. Ji, R. Lu, Cheng Guang Zhu, Zhuo Li, T. Montaruli, S. Q. Xi, Zhen Wang, Y.T. Fu, G. C. Xiao, Y. Z. Fan, X. H. Cui, Z. Y. Pei, B. D'Ettorre Piazzoli, W. X. Wu, H. Y. Jia, Y. Wang, B. Z. Dai, Alejandro Sáiz, Youping Li, J. T. Cai, R. Liu, Long Chen, Y. J. Wei, Fengqin Guo, J. F. Chang, V. Rulev, L. Xue, Liang Chen, Y. L. Xin, Yugang Zhang, Xinbo He, K. Jiang, X. J. Bi, X. J. Hu, Y. Zheng, L. Q. Yin, X. Y. Huang, J. W. Zhang, P. P. Zhang, Wenwu Tian, Pak-Hin Thomas Tam, H. C. Li, Z. X. Fan, Z. Y. You, J. Y. Yang, Ping Zhou, Junjie Mao, Y. Z. Li, F. Zheng, Y. Q. Guo, H. R. Wu, B. M. Chen, X. X. Zhou, Q. Yuan, Felix Aharonian, H. N. He, M. Heller, K. Li, L. L. Ma, Yu. V. Stenkin, Z. J. Jiang, J. Liu, Yong Zhang, R. N. Wang, C. Hou, Shuibin Lin, S. M. Liu, Lu Zhang, J. S. Wang, Cunguo Wang, E. W. Liang, N. Yin, K. J. Zhu, Minghui Liu, Shengxue Zhang, Cheng Li, Dong Liu, Jinyao Liu, C. Y. Wu, Y. M. Ye, Yunchao Liu, Y. M. Xing, H. K. Lv, X. H. Ma, Xiang Zhang, Y. Su, J. G. Guo, S. R. Zhang, M. H. Gu, L. X. Zhang, Jiawei Yan, Xin Li, and Oleg Shchegolev
Subjects: Physics, Nuclear and High Energy Physics, Photon, business.industry, Astrophysics::High Energy Astrophysical Phenomena, Astrophysics::Instrumentation and Methods for Astrophysics, Cosmic ray, Metrology, law.invention, Telescope, Air shower, Silicon photomultiplier, Optics, law, Calibration, business, Instrumentation, Cherenkov radiation
Abstract: The main scientific goal of the LHAASO WFCTA experiment is to measure the cosmic ray energy spectra and composition from 10 TeV to 1 EeV. Cherenkov photons in the extensive air shower measured by the SiPM camera of Cherenkov telescopes can be used to reconstruct the cosmic ray energy. The absolute calibration of the camera is a crucial step to achieve the accurate measurement of the cosmic ray energy spectrum. A multi-wavelength cylindrical illuminator based on LEDs is developed and mounted inside the telescope to calibrate and monitor the camera, and the illuminator’s stability is better than 0.5% under the temperature variation from -26 to 26 ° C. A portable probe with a single photoelectron resolution of 21.6% is developed. After calibration by National Institute of Metrology, China (NIM), the probe is taken to the LHAASO site to measure the absolute photon density of the cylindrical illuminator inside the telescope. Based on the illuminator with known photon density, the photon conversion factor of the camera can be calibrated, and the overall calibration uncertainty is less than 2.6%.
Published: 2022

26. Precise Measurement of the e+e− → π+π−J/ψ Cross Section at Center-of-Mass Energies from 3.77 to 4.60 GeV

Author: S. Han, Haiwen Liu, G. X. Sun, M. Savrie, J. M. Bian, Qun Ouyang, Y.N. Gao, L. Xia, Wolfgang Kuhn, P. F. Duan, A. Calcaterra, X. S. Jiang, Kanglin He, D. Y. Wang, S. H. Zhu, D. P. Jin, Xiao-Rui Lyu, H. Y. Sheng, J. S. Huang, A. Sarantsev, L. H. Wu, M. Tiemens, X. S. Qin, Xian Gao, C. Leng, M. Shao, B. L. Wang, Jianyu Zhang, L. B. Guo, D. H. Wei, E. Fioravanti, P. Musiol, C. F. Redmer, C. Schnier, Zhenyu Zhang, M. Ablikim, Yu Zhang, A. A. Zafar, B. J. Liu, Lei Zhao, X. D. Ruan, Y. J. Sun, Tao Hu, I. Tapan, Jia Liu, I. B. Nikolaev, Ding-Xiong Wang, Q. P. Ji, J. M. Zhang, R. Farinelli, Jie Zhang, L. L. Ma, L. Gong, Jingzhou Zhao, Guangshun Huang, L. Yan, Wang Zengqiang, Niu Xiaoyang, Z. Jiao, Z. J. Sun, H. L. Dai, H. X. Yang, C. Morales Morales, C. L. Luo, J. Z. Bai, Zhiqing Liu, Yuanbo Chen, Z. P. Mao, Y. P. Guo, Y. S. Zhu, Y. B. Liu, F. Feldbauer, Z. Y. You, H. H. Liu, X. L. Ji, H. H. Zhang, Michela Greco, Guangyu Zhao, J. W. Zhao, Jie Zhao, Gang Li, G. S. Varner, M. G. Zhao, Bibo Ke, Jia Xu, L. Zotti, Yuekun Heng, H. Muramatsu, J.H. Yin, H. Xiao, Hao Liang, Krisztian Peters, A. Amoroso, M. Wolke, B. Zhong, E. Boger, Lei Xu, Yongke Zhao, M. Fritsch, X. Y. Ma, Minglin Ma, L. G. Xia, M. N. Achasov, L. Yang, Xinying Song, P. Wang, D. J. Ambrose, I. Denysenko, Giulietto Felici, S. Pacetti, Xuan Zhang, N. Kalantar-Nayestanaki, Jie Liu, A. Yuncu, Chang-Zheng Yuan, Y. J. Mo, J. G. Messchendorp, Jin Li, Yingchun Zhu, M. Pelizaeus, Xiaocong Ai, Q. L. Xiu, Y. F. Wang, O. B. Kolcu, F. F. An, Y. H. Guan, F. Y. Li, R. Baldini Ferroli, A. Q. Guo, L. Fava, L. Zhang, X. R. Chen, H. Loehner, Y. F. Liang, Ming-Xing Luo, Jiajun Zheng, L. L. Wang, M. Destefanis, H. S. Chen, G. Rong, Y. T. Gu, B. Wang, J. F. Hu, T. Weber, H. Y. Zhang, Jianhao Zhang, M. Albrecht, Zheng Wang, Jianbei Liu, W. Shan, Dan Bennett, Ming Qi, X. Q. Hao, Z. Wu, Jianguo Zhang, O. Albayrak, G. A. Chelkov, Z. H. Qin, O. Bakina, M. H. Ye, S. Marcello, Talib Hussain, R. A. Briere, A. Julin, I. Uman, Chen Hu, J. F. Chang, X. K. Zhou, Y. Q. Wang, Yun-Zhi Zhang, Y. P. Lu, W. M. Song, Zhi Zeng, Y. N. Zhang, Qiang Zhao, S. Nisar, Meng Wang, X. S. Kang, Zhanwen Zhu, T. Held, Y. H. Yan, Wu Li, Xiang Li, Zhengguo Zhao, Feng Liu, Ling Zhao, Y. Ma, B. Kopf, D. M. Li, Y. Hu, T. Ma, M. Ripka, P. X. Shen, Wenbiao Yan, Kai Liu, Cunming Liu, Cui Li, N. Yu. Muchnoi, H. Cai, P. Weidenkaff, Yanwei Wang, L. D. Liu, Hong Ma, B. Y. Zhang, L. W. Jiang, Tiefu Zhao, G. Mezzadri, W. C. Yan, Xin Fang, R. Poling, G. R. Liao, X. W. Tang, S. L. Niu, M. Kornicer, Changjian Tang, X. H. Mo, W. P. Wang, Zhiqing Zhang, S. Spataro, S. S. Fang, Jingzhou Fan, D. Xiao, Li Zhou, Y. G. Xie, Yunpeng Lu, X. P. Xu, R. E. Mitchell, Y. Xia, X. K. Chu, W. J. Zheng, Shujun Zhao, J. F. Sun, Q. A. Malik, B. Kloss, D. H. Zhang, Y. Nefedov, Z. L. Dou, R. P. Guo, J. Liu, X. Y. Jiang, L. Q. Qin, F. Nerling, Zhao-Long Wang, K. Zhang, J. Lange, M. Bertani, F. A. Harris, Z. Y. Deng, M. H. Gu, W. Ikegami Andersson, X. Z. Cai, Yong Liu, D. Bettoni, Tord Johansson, C. Dong, H. J. Lu, Cunfeng Feng, Yi Fang, L. Lavezzi, K. H. Rashid, H. M. Hu, N. Qin, Lei Li, P. R. Li, Orhan Cakir, S. Sosio, Jiemin Li, Y. Z. Sun, J. L. Ping, W. X. Gong, Z. L. Hou, U. Wiedner, G. F. Xu, P. Kiese, G. Cibinetto, Siyuan Sun, Jia-ju Zhang, P. L. Liu, X. L. Luo, Y. Zhang, Zahra Haddadi, Qingnian Xu, Xiaozhong Huang, Ye-Fei Yuan, F. C. Ma, A. Denig, H. B. Liu, S. B. Liu, X. Y. Shen, Z. Gao, Mingshui Chen, Y. Pan, X. L. Kang, Q. J. Xu, Ch. Rosner, Q. W. Zhao, J. Chai, Xu Zhou, Ka-Yuet Liu, Joachim Pettersson, Andrzej Kupsc, X. C. Lou, Zhen Wang, Yiming Zhang, H. B. Li, F. De Mori, Shou-hua Zhu, Z. Liu, Fu-Hu Liu, L. J. Wu, Y. Zeng, P. Larin, F. E. Maas, W. F. Wang, S. X. Du, Cen Zhang, Teng Li, B. S. Zou, W. Gradl, X. L. Li, C. F. Qiao, J. P. Dai, S. Ahmed, Y. X. Yang, K. Schoenning, Q. Y. Li, J. V. Bennett, Niklaus Berger, K. Li, X. N. Ma, Jianbin Jiao, Y. Ding, L. S. Wang, Y. T. Liang, B. X. Yu, A. Hafner, X. H. Sun, Dmitri Dedovich, Xiang Zhou, Z. B. Li, K. Goetzen, I. Boyko, H. P. Peng, I. Garzia, B. X. Zhang, S. Z. Chen, Y. J. Mao, M. Kavatsyuk, T. Holtmann, G. F. Cao, E. H. Thorndike, Q. Gao, Fabrizio Bianchi, Q. An, J. Y. Zhang, Yuehong Xie, A. Zhemchugov, S. P. Wen, X. B. Ji, Y. Guo, Xingtao Huang, M. Y. Dong, Y. B. Li, Qingming Ma, Kai Zhu, Z. L. Huang, J. C. Chen, S. Qian, Xiang Liu, Xiaoyu Li, Jiaheng Zou, Chunxu Yu, T. J. Min, T. Luo, Junguang Lu, M. Maggiora, J. S. Yu, R. Kliemt, Guo-Ming Chen, H. Leithoff, Qi Liu, X. D. Chen, Y. H. Zheng, Fang Liu, Bingxuan Liu, H. J. Li, M. Ye, S. Jin, S. L. Olsen, C. P. Shen, Sai-Juan Chen, Jian Zhuang, M. Lara, Y. D. Wang, Wei Li, R. G. Ping, Hongji Yang, Kejun Zhu, Zhiyong Zhang, H. R. Qi, Z. J. Xiao, J. Min, C. D. Fu, Serkant Ali Cetin, P. Patteri, D. Y. Liu, Jianmin Dong, Jian Fang, Yong Ban, J. F. Qiu, S. Q. Zhang, Z. Ning, D. X. Lin, Xuejun Wang, Kai Wang, B. Zheng, Z. T. Sun, V. Prasad, L. Y. Dong, Xianglei Zhu, F. H. Heinsius, X. R. Zhou, Cheng Li, and A. Dbeyssi
Subjects: Nuclear physics, Physics, Cross section (physics), Sigma, Center of mass, Resonance (particle physics), Belle experiment, Storage ring
Abstract: The cross section for the process e(+)e(-)-> pi(+) pi(-) J/psi is measured precisely at center-of-mass energies from 3.77 to 4.60 GeV using 9 fb(-1) of data collected with the BESIII detector operating at the BEPCII storage ring. Two resonant structures are observed in a fit to the cross section. The first resonance has a mass of (222.0 +/- 3.1 +/- 1.4) MeV/ c(2) and a width of (44.1 +/- 4.3 +/- 2.0)MeV, while the second one has a mass of (4320.0 +/- 10.4 +/- 7.0)MeV/c(2) and a width of (101.4(- 19.7)(+25.3) +/- 10.2) MeV, where the first errors are statistical and second ones are systematic. The first resonance agrees with the Y(4260) resonance reported by previous experiments. The precision of its resonant parameters is improved significantly. The second resonance is observed in e(+)e(-)-> pi(+) pi(-) J/psi for the first time. The statistical significance of this resonance is estimated to be larger than 7.6 sigma. The mass and width of the second resonance agree with the Y(4360) resonance reported by the BABAR and Belle experiments within errors. Finally, the Y(4008) resonance previously observed by the Belle experiment is not confirmed in the description of the BESIII data.
Published: 2020

27. Prospects for a Multi-TeV Gamma-ray Sky Survey with the LHAASO Water Cherenkov Detector Array

Author: Guoqing Xiao, Bo Gao, Yu-Hua Yao, B. Q. Qiao, E. W. Liang, X. G. Wang, Yong Zhang, X. C. Chang, X. H. Cui, S. Wu, F. Y. Li, M. M. Ge, H. L. Dai, L. X. Bai, Z. G. Yao, Lei Zhao, Chang Jin, L. Chen, J. W. Zhao, H. D. Liu, Duo Yan, BZ Zhao, Z. X. Liu, Y. C. Nan, H. B. Li, H. K. Lv, B. D'Ettorre Piazzoli, W. X. Wu, Xiao-Yang Zhang, Y. D. Cheng, Z. H. Wang, F. R. Zhu, Y. Wang, M. Zha, P. Zhou, Yi Chen, C. X. Liu, Xufang Li, Yinong Liu, Jun-Jie Wei, Y. Y. Guo, R. Y. Liu, X. F. Wu, L. Zhang, X. J. Wang, H. M. Zhang, V. Rulev, Xiao-Hu Zhang, Y. Yu, C. Y. Wu, Zhe Cao, W. H. Huang, Guanghua Gong, Li-Sheng Geng, B. M. Chen, L. Xue, B. Liu, L. L. Yang, D. H. Huang, Y. A. Han, B. B. Zhang, D. M. Wei, Y. D. Cui, S. R. Zhang, Ziyi Wang, Zhengguo Cao, X. L. Ji, R. Lu, Jianrong Zhou, M. J. Yang, Z. Y. Pei, Y. M. Ye, S. P. Chao, H. C. Li, Jun He, Qiang Yuan, G. M. Xiang, Z. J. Jiang, Jiaxing Li, V. Alekseenko, J. F. Chang, Danzengluobu, H. Y. Jia, J. Chen, Zebo Tang, P. Pattarakijwanich, J. S. Liu, H. Y. Zhang, J. R. Mao, Wang Yanfang, H. Wang, D. Bastieri, Liang-Liang Wang, Jie Zhang, Teresa Montaruli, Cong Li, Y. Li, K. Levochkin, X. J. Bi, T. X. Zeng, Chao-Peng Wang, J. W. Zhang, S. Z. Chen, H. Liu, X. D. Sheng, Yu. V. Stenkin, C. Hou, H. Zhu, Z. K. Zeng, P. P. Zhang, P. F. Zhang, Wenwu Tian, W. J. Long, Lanqing Ma, G. G. Xin, S. H. Feng, X. Y. Wang, X. Zuo, J. C. Wang, W. H. Wang, R. Zhou, N. Yin, H. B. Hu, C. F. Feng, S. M. Liu, X. T. Huang, Yi Zhang, N. Cheng, Cheng Li, Ying Zhang, Hong-Jie Li, H. Li, Y. Zheng, M. L. Chen, Axikegu, S. B. Yang, S. W. Cui, F. Ji, J. H. Fan, Y. Z. Fan, Bo-Qiang Ma, C. W. Yang, L. Feng, Z. G. Dai, L. Z. Zhao, L. Q. Yin, Wang Yingjie, Wei Liu, Zujian Wang, Z. Li, W. Zeng, Shengxue Zhang, Q. B. Gou, Huihai He, M. H. Gu, J. Fang, X. L. Chen, H. G. Wang, O. Shchegolev, S. L. He, K. Jiang, F. Zheng, T. L. Chen, W. Gao, T. Wen, L. Shao, Yucheng Feng, M. Y. Qi, X. X. Zhou, Yiwei Wang, Felix Aharonian, K. Li, Y. F. Liang, Ruizhi Yang, Y. W. Bao, David Ruffolo, Z. Y. You, S. Hu, J. Y. Liu, Ming Chen, Warit Mitthumsiri, V. Stepanov, Q. An, Q. Gao, K. J. Zhu, Z. B. Sun, P. H. T. Tam, Y. Q. Guo, H. R. Wu, B. Z. Dai, D. Liu, M. Heller, Sina Chen, H. D. Zeng, X. H. You, Renxin Xu, C. G. Zhu, Minghui Liu, X. H. Ma, Y. He, J. R. Shi, Yuan-Ming Xing, F. F. Yang, X. X. Li, W. L. Li, Q. H. Chen, D. della Volpe, Huang Qiyan, A. Masood, H. Cai, and Alejandro Sáiz
Subjects: Nuclear and High Energy Physics, Active galactic nucleus, Cherenkov detector, media_common.quotation_subject, Astrophysics::High Energy Astrophysical Phenomena, FOS: Physical sciences, Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, 01 natural sciences, High Energy Physics - Experiment, law.invention, Hochenergie-Astrophysik Theorie - Abteilung Hinton, High Energy Physics - Experiment (hep-ex), Observatory, law, 0103 physical sciences, 010306 general physics, Instrumentation, media_common, Physics, High Energy Astrophysical Phenomena (astro-ph.HE), 010308 nuclear & particles physics, Astrophysics::Instrumentation and Methods for Astrophysics, Order (ring theory), Astronomy and Astrophysics, Projection (relational algebra), Air shower, Sky, High Energy Physics::Experiment, Astrophysics - High Energy Astrophysical Phenomena, Energy (signal processing)
Abstract: The Water Cherenkov Detector Array (WCDA) is a major component of the Large High Altitude Air Shower Array Observatory (LHAASO), a new generation cosmic-ray experiment with unprecedented sensitivity, currently under construction. The WCDA is aimed at the study of TeV $\gamma$-rays. In order to evaluate the prospects of searching for TeV $\gamma$-ray sources with the WCDA, we present in this paper a projection for the one-year sensitivity of the WCDA to TeV $\gamma$-ray sources from TeVCat (footnote: http://tevcat.uchicago.edu) using an all-sky approach. Out of 128 TeVCat sources observable to the WCDA up to a zenith angle of $45^\circ$, we estimate that 42 would be detectable for one year of observations at a median energy of 1 TeV. Most of them are Galactic sources, and the extragalactic sources are Active Galactic Nuclei (AGN)., Comment: 10 pages,10 figures, it is to be published in Chinese Physics C
Published: 2020
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28. [Analysis of influencing factors of ureteral anastomotic stenosis following urinary diversion after laparoscopic radical cystectomy]

Author: Z Y, Ye, N, Xu, S H, Chen, Y Z, Lin, S Z, Chen, D N, Chen, J B, Huang, X L, Sun, H, Cai, Q S, Zheng, Y, Wei, and X Y, Xue
Subjects: Male, Postoperative Complications, Urinary Bladder Neoplasms, Humans, Laparoscopy, Constriction, Pathologic, Urinary Diversion, Cystectomy, Retrospective Studies
Published: 2019

29. Intrinsic linearity of bakelite Resistive Plate Chambers operated in streamer mode

Author: M. Iacovacci, L. L. Ma, X. H. Ma, Hongbo Hu, X. Y. Zhang, Minghui Liu, L. Perrone, Zihuang Cao, P. Creti, Haifeng Li, R. Santonico, Yicheng Guo, J. B. Zhao, P. Salvini, A. Budano, Chang-Chun Ning, Cunfeng Feng, Zhaoyang Feng, Fudong Shi, Z. G. Yao, C. Y. Wu, B. D'Ettorre Piazzoli, H. Lu, F. R. Zhu, S. Mastroianni, Danzengluobu, G. Di Sciascio, I. De Mitri, S. M. Mari, X. C. Yang, Piero Vallania, T. L. Chen, Zhaxiciren, G. Liguori, L. Xue, Paolo Camarri, Zhenyong Feng, B. Bartoli, C. X. Liu, H. W. Wang, Zhaxisangzhu, J. K. K. Liu, H. Y. Jia, Longzhou Zhang, Q. Q. Zhu, M. Zha, X. J. Bi, M. Panareo, G. Mancarella, S. W. Cui, S. Z. Chen, T. Di Girolamo, H. R. Wu, B. Z. Dai, F. Ruggieri, P. Branchini, Q. B. Gou, A. F. Yuan, Labaciren, Q. Y. Yang, G. Zizzi, H. H. He, Y. H. Tan, A. D'Amone, X. D. Sheng, Paolo Bernardini, Paolo Montini, R. Iuppa, R. Cardarelli, G. Marsella, S. Vernetto, Pengnian Shen, S. Catalanotti, P. Pistilli, H. M. Zhang, X. X. Zhou, A. Surdo, Carlo Vigorito, Haibing Hu, Y. Zhang, D. Martello, Bartoli B., Bernardini P., Bi X. J., Branchini P., Budano A., Camarri P., Cao Z., Cardarelli R., Catalanotti S., Chen S. Z., Chen T. L., Creti P., Cui S. W., Dai B. Z., D'Amone A., Danzengluobu, De Mitri I., D'Ettorre Piazzoli B., Di Girolamo T., Di Sciascio G., Feng C. F., Feng Z., Gou Q. B., Guo Y. Q., He H. H., Hu H., Iacovacci M., Iuppa R., Jia H. Y., Labaciren, Li H. J., Liguori G., Liu C., Liu J., Liu M. Y., Lu H., Ma L. L., Ma X. H., Mancarella G., Mari S. M., Marsella G., Martello D., Mastroianni S., Montini P., Ning C. C., Panareo M., Perrone L., Pistilli P., Ruggieri F., Salvini P., Santonico R., Shen P. R., Sheng X. D., Shi F., Surdo A., Tan Y. H., Vallania P., Vernetto S., Vigorito C., Wang H., Wu C. Y., Wu H. R., Xue L., Yang Q. Y., Yang X. C., Yao Z. G., Yuan A. F., Zha M., Zhang H. M., Zhang L., Zhang X. Y., Zhang Y., Zhao J., Zhaxiciren Zhaxisangzhu, Zhou X. X., Zhu F. R., Zhu Q. Q., Zizzi G., Bartoli, B., Bernardini, P., Bi, X. J., Branchini, P., Budano, A., Camarri, P., Cao, Z., Cardarelli, R., Catalanotti, S., Chen, S. Z., Chen, T. L., Creti, P., Cui, S. W., Dai, B. Z., D'Amone, A., De Mitri, I., D'Ettorre Piazzoli, B., Di Girolamo, T., Di Sciascio, G., Feng, C. F., Feng, Z., Gou, Q. B., Guo, Y. Q., He, H. H., Hu, H., Iacovacci, M., Iuppa, R., Jia, H. Y., Li, H. J., Liguori, G., Liu, C., Liu, J., Liu, M. Y., Lu, H., Ma, L. L., Ma, X. H., Mancarella, G., Mari, S. M., Marsella, G., Martello, D., Mastroianni, S., Montini, P., Ning, C. C., Panareo, M., Perrone, L., Pistilli, P., Ruggieri, F., Salvini, P., Santonico, R., Shen, P. R., Sheng, X. D., Shi, F., Surdo, A., Tan, Y. H., Vallania, P., Vernetto, S., Vigorito, C., Wang, H., Wu, C. Y., Wu, H. R., Xue, L., Yang, Q. Y., Yang, X. C., Yao, Z. G., Yuan, A. F., Zha, M., Zhang, H. M., Zhang, L., Zhang, X. Y., Zhang, Y., Zhao, J., Zhaxiciren, Zhaxisangzhu, Zhou, X. X., Zhu, F. R., Zhu, Q. Q., Zizzi, G., D’Amone, A., Danzengluobu, Null, D’Ettorre Piazzoli, B., Feng, Zhaoyang, Feng, Zhenyong, Hu, Haibing, Hu, Hongbo, Labaciren, Null, Zhaxiciren, Null, and Zhaxisangzhu, Null
Subjects: Nuclear and High Energy Physics, Physics::Instrumentation and Detectors, Intrinsic linearity, Streamer mode, Cosmic ray, Calorimetry, 01 natural sciences, chemistry.chemical_compound, Optics, 0103 physical sciences, Bakelite, Particle density, 010303 astronomy & astrophysics, Instrumentation, Physics, Resistive touchscreen, 010308 nuclear & particles physics, business.industry, Detector, Settore FIS/01 - Fisica Sperimentale, Linearity, RPC detector, Streamer mode, Intrinsic linearity, Calorimetry, chemistry, Particle, Physics::Accelerator Physics, RPC detector, business, Beam (structure)
Abstract: Resistive Plate Chambers have largely been used in High Energy Physics and Cosmic Ray research. In view of using this detector for calorimetry applications it is important to know the maximum measurable particle density, or its intrinsic linearity limit, which is tightly related to the dimension of the discharge region. In this paper we report the results of measurements performed at the Beam Test Facility (INFN National Laboratory of Frascati, Italy) where the intrinsic linearity of bakelite RPCs operated in streamer mode has been tested at different impinging particle densities.
Published: 2019

30. [Effectiveness of snail control by immersion of molluscicides through tide diversion in marshlands: a field evaluation]

Author: Q L, Qiu, S Z, Chen, Y P, Zuo, K, Tang, G L, Du, and Y X, Huang
Subjects: Molluscacides, Suspensions, Surveys and Questionnaires, Wetlands, Immersion, Snails, Animals, Niclosamide, Pest Control, Tidal Waves
Abstract: To compare the effectiveness of snail control between immersion of molluscicides through tide diversion and mollusciciding by spraying in marshland areas.Immersion of 26% suspension concentrate of metaldehyde and niclosamide through tide diversion and spraying 26% suspension concentrate of metaldehyde and niclosamide alone were employed for snail control in two neighboring snail-breeding marshlands, and snails were surveyed before and after mollusciciding. The mortality of snails and the density of living snails were estimated.The density of living snails reduced by 72.19% and 100.00% 1 and 2 years after immersion of 26% suspension concentrate of metaldehyde and niclosamide through tide diversion, and 5.93% and 18.15% 1 and 2 years after spraying 26% suspension concentrate of metaldehyde and niclosamide alone.Immersion of 26% suspension concentrate of metaldehyde and niclosamide through tide diversion is significantly superior to spraying 26% suspension concentrate of metaldehyde and niclosamide along for snail control, and implementation of immersion of 26% suspension concentrate of metaldehyde and niclosamide through tide diversion for more than 2 successive years may achieve a higher snail control efficiency.
Published: 2019

31. Calibration of the LHAASO-KM2A electromagnetic particle detectors using charged particles within the extensive air showers

Author: Ye Liu, Z. M. Zhang, Sha Wu, Hongkui Lv, Huihai He, S. Z. Chen, Yaping Wang, Jing Zhao, C. Hou, Jia Liu, and Xiangdong Sheng
Subjects: Physics, Physics::Instrumentation and Detectors, 010308 nuclear & particles physics, Monte Carlo method, Detector, Astrophysics::Instrumentation and Methods for Astrophysics, Astronomy and Astrophysics, Cosmic ray, 01 natural sciences, Charged particle, Air shower, Observatory, 0103 physical sciences, Calibration, Particle, 010303 astronomy & astrophysics, Remote sensing
Abstract: In the Large High Altitude Air Shower Observatory (LHAASO), one square kilometer array (KM2A), with 5242 electromagnetic particle detectors (EDs) and 1171 muon detectors (MDs), is designed to study ultra-high energy gamma-ray astronomy and cosmic ray physics. The remoteness and numerous detectors extremely demand a robust and automatic calibration procedure. In this paper, a self-calibration method which relies on the measurement of charged particles within the extensive air showers is proposed. The method is fully validated by Monte Carlo simulation and successfully applied in a KM2A prototype array experiment. Experimental results show that the self-calibration method can be used to determine the detector time offset constants at the sub-nanosecond level and the number density of particles collected by each ED with an accuracy of a few percents, which are adequate to meet the physical requirements of LHAASO experiment. This software calibration also offers an ideal method to realtime monitor the detector performances for next generation ground-based EAS experiments covering an area above square kilometers scale.
Published: 2018

32. A calibration of WFCTA prototype telescopes using N2 laser

Author: M. H. Gu, G. C. Xiao, S. H. Feng, Zihuang Cao, M. Zha, L. L. Ma, M. J. Chen, Bin Zhou, J. Liu, X. Zuo, H. Y. Jia, Bai Yibing, Bingshui Gao, Shengxue Zhang, C. Hou, J. B. Zhao, S. Z. Chen, B.K. Zhang, H. H. He, Y. Zhang, Jiali Liu, and F. R. Zhu
Subjects: Physics, Nuclear and High Energy Physics, Photon, 010308 nuclear & particles physics, business.industry, Scattering, Aperture, Detector, Astrophysics::Instrumentation and Methods for Astrophysics, Field of view, Laser, 01 natural sciences, law.invention, 010309 optics, Telescope, Optics, law, 0103 physical sciences, Calibration, business, Instrumentation
Abstract: An end-to-end calibration method, which is different from the traditional way, has been employed in WFCTA prototype experiment based on N 2 laser. As we known, the calculation of the expected and the observed light fluxes at the front of the aperture of the telescope are crucial in the such method. To calculate predicted light flux accurately, the propagation and scattering of photons in the atmosphere have been considered in detail. In order to get the detector effective areas, which will be used in the transformation of ADC signals to the observed light flux, a ray trace procedure, considering all details of detector response, has been performed for all incident direction of photons in field of view of the detector. By matching the observed and expected light flux at the entrance of the telescope, the overall calibration gains of two telescopes can be obtained. During the test run of the calibration, a overall calibration gain around G = 0 . 38 A D C c o u n t s ∕ p h o t o n and G = 0 . 36 A D C c o u n t s ∕ p h o t o n for WFCT01 and WFCT02 are given, respectively. Furthermore, in view of all uncertainty sources, systematic uncertainties for the calibration have also been estimated. They are around the level of ( − 7 . 3 % , + 7 . 8 % ) . The calibration results achieved by end-to-end method and the traditional way are in consistent at the level of 10%, which is within the range of uncertainties. Since the end-to-end and traditional calibration methods have their own advantages, the performance of the combination of these two calibration methods has also been discussed in the end.
Published: 2018

33. Geometrical reconstruction of fluorescence events observed by the LHAASO experiment *

Author: F. Aharonian, Q. An, null Axikegu, L. X. Bai, Y. X. Bai, Y. W. Bao, D. Bastieri, X. J. Bi, Y. J. Bi, H. Cai, J. T. Cai, Z. Cao, J. Chang, J. F. Chang, X. C. Chang, B. M. Chen, J. Chen, L. Chen, M. J. Chen, M. L. Chen, Q. H. Chen, S. H. Chen, S. Z. Chen, T. L. Chen, X. L. Chen, Y. Chen, N. Cheng, Y. D. Cheng, S. W. Cui, X. H. Cui, Y. D. Cui, B. Z. Dai, H. L. Dai, Z. G. Dai, null Danzengluobu, D. della Volpe, B. D'Ettorre Piazzoli, X. J. Dong, J. H. Fan, Y. Z. Fan, Z. X. Fan, J. Fang, K. Fang, C. F. Feng, L. Feng, S. H. Feng, Y. L. Feng, B. Gao, C. D. Gao, Q. Gao, W. Gao, M. M. Ge, L. S. Geng, G. H. Gong, Q. B. Gou, M. H. Gu, J. G. Guo, X. L. Guo, Y. Q. Guo, Y. Y. Guo, Y. A. Han, H. H. He, H. N. He, J. C. He, S. L. He, X. B. He, Y. He, M. Heller, Y. K. Hor, C. Hou, X. Hou, H. B. Hu, S. Hu, S. C. Hu, X. J. Hu, D. H. Huang, Q. L. Huang, W. H. Huang, X. T. Huang, Z. C. Huang, F. Ji, X. L. Ji, H. Y. Jia, K. Jiang, Z. J. Jiang, C. Jin, D. Kuleshov, K. Levochkin, B. B. Li, C. Li, F. Li, H. B. Li, H. C. Li, H. Y. Li, J. Li, K. Li, W. L. Li, X. Li, X. R. Li, Y. Li, Y. Z. Li, Z. Li, E. W. Liang, Y. F. Liang, S.J. Lin, B. Liu, C. Liu, D. Liu, H. Liu, H. D. Liu, J. Liu, J. L. Liu, J. S. Liu, J. Y. Liu, M. Y. Liu, R. Y. Liu, S. M. Liu, W. Liu, Y. N. Liu, Z. X. Liu, W. J. Long, R. Lu, H. K. Lv, B. Q. Ma, L. L. Ma, X. H. Ma, J. R. Mao, A. Masood, W. Mitthumsiri, T. Montaruli, Y. C. Nan, B. Y. Pang, P. Pattarakijwanich, Z. Y. Pei, M. Y. Qi, D. Ruffolo, V. Rulev, A. Sáiz, L. Shao, O. Shchegolev, X. D. Sheng, J. R. Shi, H. C. Song, Yu.V. Stenkin, V. Stepanov, Q. N. Sun, X. N. Sun, Z. B. Sun, P. H. T. Tam, Z. B. Tang, W. W. Tian, B. D. Wang, C. Wang, H. Wang, H. G. Wang, J. C. Wang, J. S. Wang, L. P. Wang, L. Y. Wang, R. N. Wang, W. Wang, X. G. Wang, X. J. Wang, X. Y. Wang, Y. D. Wang, Y. J. Wang, Y. P. Wang, Z. Wang, Z. H. Wang, Z. X. Wang, D. M. Wei, J. J. Wei, Y. J. Wei, T. Wen, C. Y. Wu, H. R. Wu, S. Wu, W. X. Wu, X. F. Wu, S. Q. Xi, J. Xia, J. J. Xia, G. M. Xiang, G. Xiao, H. B. Xiao, G. G. Xin, Y. L. Xin, Y. Xing, D. L. Xu, R. X. Xu, L. Xue, D. H. Yan, C. W. Yang, F. F. Yang, J. Y. Yang, L. L. Yang, M. J. Yang, R. Z. Yang, S. B. Yang, Y. H. Yao, Z. G. Yao, Y. M. Ye, L. Q. Yin, N. Yin, X. H. You, Z. Y. You, Y. H. Yu, Q. Yuan, H. D. Zeng, T. X. Zeng, W. Zeng, Z. K. Zeng, M. Zha, X. X. Zhai, B. B. Zhang, H. M. Zhang, H. Y. Zhang, J. L. Zhang, J. W. Zhang, L. Zhang, L. X. Zhang, P. F. Zhang, P. P. Zhang, R. Zhang, S. R. Zhang, S. S. Zhang, X. Zhang, X. P. Zhang, Y. Zhang, Y. F. Zhang, Y. L. Zhang, B. Zhao, J. Zhao, L. Zhao, L. Z. Zhao, S. P. Zhao, F. Zheng, Y. Zheng, B. Zhou, H. Zhou, J. N. Zhou, P. Zhou, R. Zhou, X. X. Zhou, C. G. Zhu, F. R. Zhu, H. Zhu, K. J. Zhu, and X. Zuo
Subjects: Physics, Nuclear and High Energy Physics, Physics::Instrumentation and Detectors, 010308 nuclear & particles physics, business.industry, Astrophysics::High Energy Astrophysical Phenomena, Detector, Resolution (electron density), Astrophysics::Instrumentation and Methods for Astrophysics, Astronomy and Astrophysics, Cosmic ray, 01 natural sciences, Fluorescence, law.invention, Telescope, Optics, law, 0103 physical sciences, Trajectory, Range (statistics), 010306 general physics, business, Instrumentation, Cherenkov radiation
Abstract: The LHAASO-WFCTA experiment, which aims to observe cosmic rays in the sub-EeV range using the fluorescence technique, uses a new generation of high-performance telescopes. To ensure that the experiment has excellent detection capability associated with the measurement of the energy spectrum, the primary composition of cosmic rays, and so on, an accurate geometrical reconstruction of air-shower events is fundamental. This paper describes the development and testing of geometrical reconstruction for stereo viewed events using the WFCTA (Wide Field of view Cherenkov/Fluorescence Telescope Array) detectors. Two approaches, which take full advantage of the WFCTA detectors, are investigated. One is the stereo-angular method, which uses the pointing of triggered SiPMs in the shower trajectory, and the other is the stereo-timing method, which uses the triggering time of the fired SiPMs. The results show that both methods have good geometrical resolution; the resolution of the stereo-timing method is slightly better than the stereo-angular method because the resolution of the latter is slightly limited by the shower track length.
Published: 2021

34. Investigation on the Effect of Dead Time on the Phase of Fundamental Voltage in VSI-PMSM Drive System

Author: J. F. Jiang and S. Z. Chen
Subjects: Computer science, Control theory, Phase (waves), Dead time, Voltage
Abstract: Both electric vehicle PMSM drive system and grid connected photovoltaic (PV) power generation need voltage source inverter (VSI). The dead time should be set properly when the power switches are turned on and off in the same bridge arm of VSI. During the dead time, the load is out of control, which will cause the abnormal output voltage amplitude and phase. However the influence of dead time on the output fundamental voltage phase has not been paid much attention to and studied. Firstly, in the paper, the phase shift of output fundamental voltage caused by dead time is simulated and analyzed for three-phase VSI - resistance inductance series (RL) load system under several conditions such as variable switching frequency, modulation index, output fundamental frequency and dead time. Secondly, take three-phase VSI - permanent magnet synchronous motor (PMSM) drive system for instance, the simulation analysis of output fundamental voltage phase shift and rotor positioning error caused by dead time are also performed, and an off-line method to compensate the fundamental voltage phase based on αβ coordinate is given. The above work provides a reference for further understanding the influence of dead time on fundamental voltage phase shift in VSI, so as to improve the monitoring and control precision of electric vehicle drive system. The analysis approach can be applicable to the grid connected photovoltaic (PV) power generation PMSM servo system.
Published: 2021

35. Study of J/ψ and ψ(3686)→Σ(1385)0Σ¯(1385)0 and Ξ0Ξ¯0

Author: Tao Luo, X. N. Ma, Y. T. Liang, F. De Mori, X. Y. Zhou, F. E. Maas, M. Fritsch, H. H. Liu, J. C. Li, B. X. Yu, T. Hu, S. L. Niu, Zhi Zeng, J. Zhuang, M. Kavatsyuk, F. Y. Li, R. Farinelli, Xiao-Rui Lyu, Z. J. Xiao, X. Q. Li, Y. F. Long, M. X. Luo, G. S. Varner, Zhiqing Liu, C. Hu, M. Maggiora, Ling Zhao, M. Greco, O. Bakina, D. V. Dedovich, X. F. Wang, Minglin Ma, X. Tang, J. Min, T. Johansson, J. F. Chang, H. S. Chen, Lei Zhao, Z. L. Hou, B. X. Zhang, H. L. Ma, D. M. Li, G. F. Xu, Q. M. Ma, O. B. Kolcu, X. Cai, S. Jin, P. X. Shen, H. L. Dai, Igor Boyko, Y. Ding, B. Kopf, M. Y. Dong, Z. Wu, B. J. Liu, K. L. He, B. Kloss, X. Y. Niu, Y. Yuan, L. W. Jiang, Y. S. Zhu, C. Z. Yuan, X. Q. Hao, K. Y. Liu, M. Pelizaeus, Y. B. Zhao, Y. Guo, M. Z. Wang, Xiaozhong Huang, Z. B. Li, W. Ikegami Andersson, Q. Ouyang, Jimin Zhao, Zhiqing Zhang, S. S. Fang, X. Y. Song, K. J. Zhu, W. Shan, Y. H. Zheng, Cong-Feng Qiao, O. Albayrak, T. Holtmann, J. Dong, W. Kühn, J. M. Bian, Z. Y. You, Z. A. Zhu, Bingxuan Liu, Yao Wang, Y. Q. Wang, Q. Liu, Andrzej Kupsc, M. Qi, H. J. Yang, Guangshun Huang, S. Nisar, L. Yan, R. Baldini Ferroli, X. D. Ruan, Y. B. Liu, Z. H. Wang, K. Goetzen, L. L. Ma, L. Gong, C. J. Tang, Y. Hu, Y. P. Lu, B. Wang, A. Calcaterra, Z. G. Zhao, P. L. Wang, X. L. Gao, M. L. Chen, S. J. Zhao, N. Yu. Muchnoi, X. S. Kang, Y. H. Zhang, J. Y. Liu, Y. H. Guan, H. B. Liu, W. G. Li, Q. P. Ji, S. Spataro, X. P. Xu, Y. F. Wang, G. Li, L. Zotti, L. G. Xia, Kai Liu, Y. Y. Liu, C. Leng, P. Musiol, C. F. Redmer, Xiaocong Ai, Lei Li, C. Schnier, D. Xiao, Q. A. Malik, C. Dong, S. Sosio, X. L. Luo, A. Amoroso, C. P. Shen, A. Dbeyssi, F. A. Harris, W. P. Wang, S. B. Liu, M. Kornicer, F. Bianchi, X. Y. Ma, J. H. Zou, M. Bertani, Q. J. Xu, W. X. Gong, Z. Haddadi, Jun-Yi Zhang, Y. P. Guo, Z. P. Zhang, H. H. Zhang, J. C. Chen, X. T. Huang, Z. J. Sun, H. Loehner, Yu Zhang, Magnus Wolke, Y. F. Liang, A. A. Zafar, Q. Gao, Z. Ning, L. Yang, L. J. Wu, Joachim Pettersson, Y. N. Gao, H. M. Liu, Y. Zhang, X. N. Li, C. D. Fu, Z. Y. Wang, C. Q. Feng, X. R. Chen, Y. J. Mo, Z. Y. Deng, A. Julin, Xuanhong Lou, Haiping Peng, G. F. Cao, G. Mezzadri, X. Fang, S. S. Sun, G. Rong, Nasser Kalantar-Nayestanaki, D. P. Jin, Y. Nefedov, Q. An, J. H. Liu, W. C. Yan, Z. L. Huang, Feng Liu, Ke Wang, J. J. Xu, G. R. Liao, Xingguo Li, X. H. Sun, D. W. Bennett, Zujian Wang, J. Z. Fan, A. Zhemchugov, C. Morales Morales, Dayong Wang, N. Qin, T. Weber, Y. J. Mao, Y. B. Li, H. X. Yang, M. Ablikim, Z. G. Wang, H. Y. Zhang, P. F. Duan, E. H. Thorndike, J. Q. Zhang, W. Gradl, I. Garzia, M. Ripka, J. S. Huang, H. B. Li, A. G. Denig, C. L. Luo, J. Z. Bai, X. Y. Jiang, C. X. Liu, G. F. Chen, C. C. Zhang, P. Kiese, G. Felici, Yunlong Zhang, Gianfranco Morello, Fenfen An, L. Q. Qin, B. L. Wang, D. Y. Wang, J. Y. Zhang, F. Feldbauer, B. Zhong, L. B. Guo, S. L. Olsen, R. A. Briere, X. B. Ji, M. Tiemens, S. Ahmed, Y. X. Yang, T. C. Zhao, X. S. Jiang, D. Bettoni, Liqing Xu, Cui Li, J. L. Zhang, P. Patteri, X. Y. Shen, R. Poling, X. C. Chen, H. Muramatsu, Ulrich Wiedner, R. Kliemt, Klaus Peters, L. P. Zhou, J. P. Liu, Y. Pan, J. Chai, Y. K. Heng, H. Leithoff, G. X. Sun, J. V. Bennett, Y. M. Ma, J. G. Messchendorp, Jie Yu, H. J. Li, Jin Li, J. P. Dai, Q. L. Xiu, T. J. Min, Jianping Zheng, S. Zhu, F. Li, T. Ma, Z. Jiao, Fu-Hu Liu, D. H. Zhang, F. C. Ma, O. Cakir, R. E. Mitchell, G. Cibinetto, A. Hafner, Qiunan Xu, S. J. Chen, Z. P. Mao, Q. Zhao, Y. Z. Sun, M. G. Zhao, R. P. Guo, Y. H. Xie, A. Q. Guo, J. Fang, Tao Li, Y. N. Zhang, Xiang Zhou, J. F. Qiu, L. Fava, Gang Zhao, S. Han, J. J. Zhang, M. Destefanis, W. M. Song, Z. Gao, Y. X. Xia, S. H. Zhu, Bibo Ke, L. H. Wu, Ch. Rosner, M. Savrie, Z. H. Qin, L. Xia, H. Liang, W. B. Yan, M. N. Achasov, I. B. Nikolaev, I. Uman, S. Pacetti, P. Larin, D. J. Ambrose, J. F. Sun, S. Z. Chen, M. Albrecht, S. Marcello, W. D. Li, Y. Zeng, Yaquan Fang, Jie Zhao, D. X. Lin, H. M. Hu, K. Li, X. K. Zhou, Fang Liu, I. Tapan, K. Schoenning, Q. Y. Li, B. S. Zou, Y. H. Yan, J. W. Zhang, Y. B. Chen, Xiaofeng Zhu, J. Z. Zhang, J. W. Zhao, I. Denysenko, Niklaus Berger, Y. C. Zhu, B. Y. Zhang, H. Xiao, T. Held, X. Liu, H. R. Qi, Serkant Ali Cetin, D. Y. Liu, J. B. Jiao, S. Q. Zhang, S. Qian, Jialun Ping, K. Zhang, X. Y. Zhang, M. Lara, J. B. Liu, Y. J. Sun, E. Boger, M. H. Gu, H. Y. Sheng, C. X. Yu, B. Zheng, R. G. Ping, X. L. Ji, Z. T. Sun, G. A. Chelkov, Talib Hussain, Z. A. Liu, V. Prasad, Yanwei Wang, A. Yuncu, Y. G. Xie, Y. Ban, P. Weidenkaff, F. H. Heinsius, S. X. Du, Z. L. Dou, S. P. Wen, X. S. Qin, X. R. Zhou, Cheng Li, X. K. Chu, M. H. Ye, Peilian Liu, Lingxuan Zhang, Zhiyong Zhang, L. D. Liu, L. Y. Dong, W. J. Zheng, F. Nerling, J. H. Yin, K. H. Rashid, M. Shao, Y. T. Gu, E. Fioravanti, X. L. Kang, A. Sarantsev, D. H. Wei, P. R. Li, J. S. Lange, Q. W. Zhao, X. H. Mo, L. S. Wang, L. L. Wang, H. Cai, H. J. Lu, and J. G. Lu
Subjects: Baryon, Nuclear physics, Physics, Nuclear and High Energy Physics, Particle physics, Angular distribution, 010308 nuclear & particles physics, Branching fraction, Isospin, Electron–positron annihilation, 0103 physical sciences, 010306 general physics, 01 natural sciences
Abstract: We study the decays of J / ψ and ψ ( 3686 ) to the final states Σ ( 1385 ) 0 Σ ¯ ( 1385 ) 0 and Ξ 0 Ξ ¯ 0 based on a single baryon tag method using data samples of ( 1310.6 ± 7.0 ) × 10 6 J / ψ and ( 447.9 ± 2.9 ) × 10 6 ψ ( 3686 ) events collected with the BESIII detector at the BEPCII collider. The decays to Σ ( 1385 ) 0 Σ ¯ ( 1385 ) 0 are observed for the first time. The measured branching fractions of J / ψ and ψ ( 3686 ) to Ξ 0 Ξ ¯ 0 are in good agreement with, and much more precise than, the previously published results. The angular parameters for these decays are also measured for the first time. The measured angular decay parameter for J / ψ → Σ ( 1385 ) 0 Σ ¯ ( 1385 ) 0 , α = − 0.64 ± 0.03 ± 0.10 , is found to be negative, different to the other decay processes in this measurement. In addition, the “12% rule” and isospin symmetry in the decays of J / ψ and ψ ( 3686 ) to Ξ Ξ ¯ and Σ ( 1385 ) Σ ¯ ( 1385 ) are tested.
Published: 2017

36. Absolute-energy-scale calibration of ARGO-YBJ for light primaries in multi-TeV region with the Moon shadow observation

Author: X. C. Yang, H. H. He, T. Di Girolamo, Zhenyong Feng, H. Y. Jia, B. D'Ettorre Piazzoli, L. Xue, Hong-peng Lu, P. Pistilli, H. M. Zhang, X. X. Zhou, M. Iacovacci, M. Zha, Labaciren, X. D. Sheng, S. M. Mari, J. K. K. Liu, A. Surdo, Paolo Bernardini, L. L. Ma, Haibing Hu, Longzhou Zhang, H. W. Wang, J. B. Zhao, P. Salvini, Chang-Chun Ning, C. X. Liu, H. J. Li, H. R. Wu, Zhaoyang Feng, G. Marsella, X. J. Bi, Y. Zhang, Z. G. Yao, G. Mancarella, Zhaxisangzhu, C. Y. Wu, B. Bartoli, S. Z. Chen, L. Perrone, R. Santonico, G. Di Sciascio, Y. H. Tan, Fudong Shi, B. Z. Dai, S. Mastroianni, Carlo Vigorito, Zhaxiciren, F. R. Zhu, Danzengluobu, Y. Q. Guo, Q. Q. Zhu, I. De Mitri, Q. B. Gou, Zihuang Cao, Piero Vallania, T. L. Chen, A. F. Yuan, Pengnian Shen, S. Catalanotti, S. W. Cui, Hongbo Hu, C. F. Feng, P. Montini, X. H. Ma, X. Y. Zhang, Minghui Liu, R. Iuppa, S. Vernetto, A. D'Amone, Q. Y. Yang, Bartoli, B., Bernardini, P., Bi, X. J., Cao, Z., Catalanotti, S., Chen, S. Z., Chen, T. L., Cui, S. W., Dai, B. Z., D'Amone, A., Danzengluobu, Null, De Mitri, I., D'Ettorre Piazzoli, B., Di Girolamo, T., Di Sciascio, G., Feng, C. F., Feng, Zhaoyang, Feng, Zhenyong, Gou, Q. B., Guo, Y. Q., He, H. H., Hu, Haibing, Hu, Hongbo, Iacovacci, M., Iuppa, R., Jia, H. Y., Labaciren, Null, Li, H. J., Liu, C., Liu, J., Liu, M. Y., Lu, H., Ma, L. L., Ma, X. H., Mancarella, G., Mari, Stefano Maria, Marsella, G., Mastroianni, S., Montini, Paolo, Ning, C. C., Perrone, L., Pistilli, Pio, Salvini, P., Santonico, R., Shen, P. R., Sheng, X. D., Shi, F., Surdo, A., Tan, Y. H., Vallania, P., Vernetto, S., Vigorito, C., Wang, H., Wu, C. Y., Wu, H. R., Xue, L., Yang, Q. Y., Yang, X. C., Yao, Z. G., Yuan, A. F., Zha, M, Zhang, H. M., Zhang, L., Zhang, X. Y., Zhang, Y., Zhao, J., Zhaxiciren, Null, Zhaxisangzhu, Null, Zhou, X. X., Zhu, F. R., Zhu, Q. Q., Bernardini, Paolo, D'Amone, Antonio, DE MITRI, Ivan, D’Ettorre Piazzoli, B., Mancarella, Giovanni, Mari, S. M., Marsella, Giovanni, Montini, P., Perrone, Lorenzo, Pistilli, P., Zha, M., and collaboration), (The ARGO YBJ
Subjects: Cosmic ray, Energy calibration, Energy spectrum, Moon shadow, Physics, Large Hadron Collider, 010308 nuclear & particles physics, Astrophysics::High Energy Astrophysical Phenomena, Hadron, Moon shadow, Astronomy, Astronomy and Astrophysics, Cosmic ray, Interaction model, Astrophysics, 01 natural sciences, Scale error, Energy calibration, Energy spectrum, Rigidity (electromagnetism), 0103 physical sciences, Ultra-high-energy cosmic ray, 010303 astronomy & astrophysics, Argo
Abstract: In 2011 ARGO-YBJ experiment has reported a work to study the absolute rigidity scale of the primary cosmic ray particles based on the Moon's shadow observation. Given the progress in high energy hadronic interaction models with LHC data, in cosmic ray chemical composition measurement and in experimental data accumulation, more updates can be researched. This paper aims to further disentangle the composition dependence in absolute-energy-scale calibration by using specific moon-shadow data which mainly is comprised of light component cosmic rays. Results show that, 17% energy scale error is estimated from 3 TeV to 50 TeV. To validate the performance of this technique, the light component cosmic ray spectrum in the same energy region is shown. (C) 2017 Elsevier B.V. All rights reserved.
Published: 2017

37. The expectation of LHAASO sensitivity on the cosmic-ray electron

Author: Huihai He, Sujie Lin, Yuncheng Nan, Sha Wu, and S. Z. Chen
Subjects: Physics, Nuclear physics, Energy loss, Astrophysics::High Energy Astrophysical Phenomena, Background suppression, Dark matter, Hadron, Dipole anisotropy, Cosmic ray, Electron, Sensitivity (control systems)
Abstract: The high-energy electrons suffer severe energy loss during their propagation, owing to the Syn chrotron and Inverse-Compton processes. Thus, the electrons exceeding TeV are most likely originating from few local sources, such as dark matter particle and astrophysical sources. The dipole anisotropy of the electrons is also regard as an unique signature about the nearby sources. With the merit of large detecting area and strong background suppression, the LHAASO exper iment provides an opportunity on extending the detection of high-energy cosmic-ray electrons from 500 GeV to 100 TeV. In this paper, We explore the efficient rejection of hadronic back ground of LHAASO, in combination with KM2A and WCDA and make the expectation on the spectrum of cosmic-ray electrons and the sensitivity of dipole anisotropy with LHAASO. The influence on the research of electronic origin is also discussed.
Published: 2019

38. Estimation of solar disk gamma-ray emission based on Geant4

Author: Cong Li, Yuncheng Nan, Zhe Li, S. Z. Chen, and Huihai He
Subjects: Physics, Astrophysics::High Energy Astrophysical Phenomena, Physics::Space Physics, Gamma ray, Astrophysics::Solar and Stellar Astrophysics, Flux, Cosmic ray, Astrophysics::Earth and Planetary Astrophysics, Solar atmosphere, Solar disk, Computational physics, Fermi Gamma-ray Space Telescope, Magnetic field
Abstract: The most important astrophysical mechanism for steady solar gamma-ray emission is the interaction of cosmic rays with solar atmosphere, which has been definitely detected by Fermi-LAT with maximum energy up to 200 GeV. Some studies shown that the effect of the solar magnetic field to solar disk gamma-ray flux is unneglectable. It is valuable to study the physical mechanism between solar disk gamma-ray flux and solar magnetic field. In this paper, we simulated the interaction between cosmic rays and solar atmosphere by G4SOLAR program based on Geant4. A simulated solar disk gamma-ray flux from 1GeV to 1TeV was obtained with taking into account the influence of coronal magnetic field. The PFSS model for “quiet”Sun was employed, and the solar disk gamma-ray below 10GeV was consistent with the Fermi observation. But the simulated spectrum became much softer than Fermi data when >10GeV. Some influence factors were briefly discussed.
Published: 2019

39. Search for Gamma-Ray Emission from the Sun during Solar Minimum with the ARGO-YBJ Experiment

Author: C. Y. Wu, Labaciren, Q. Y. Yang, P. Montini, X. H. Ma, C. C. Ning, Haifeng Li, C. Q. Liu, Q. B. Gou, Q. Q. Zhu, L. Zhang, T. L. Chen, Danzengluobu, C. Vigorito, P. Bernardini, R. Santonico, Zhaxisangzhu, Hongbo Hu, Yicheng Guo, A. Surdo, Y. H. Tan, P. R. Shen, X. C. Yang, H. Y. Jia, H. R. Wu, S. Catalanotti, B. Z. Dai, J. Zhao, Huihai He, Zhaoyang Feng, F. R. Zhu, P. Pistilli, H. M. Zhang, H. Lu, Minghui Liu, G. Di Sciascio, X. Y. Zhang, Zihou Li, G. Mancarella, I. De Mitri, T. Di Girolamo, Zhaxiciren, Xiangdong Sheng, R. Iuppa, S. W. Cui, A. F. Yuan, S. Vernetto, S. Z. Chen, A. D'Amone, Cunfeng Feng, H. Wang, S. Mastroianni, Y. J. Zhang, Haibing Hu, B. Bartoli, X. J. Bi, L. Perrone, J. K. K. Liu, L. L. Ma, W. Gao, M. Zha, Zhenyong Feng, X. X. Zhou, P. Vallania, B. D'Ettorre Piazzoli, L. Xue, Z. G. Yao, M. Iacovacci, Zhengguo Cao, F. Shi, P. Salvini, G. Marsella, S. M. Mari, Bartoli B., Bernardini P., Bi X. J., Cao Z., Catalanotti S., Chen S. Z., Chen T. L., Cui S. W., Dai B. Z., D'Amone A., Danzengluobu, Mitri I. D., Piazzoli B. D., Girolamo T. D., Sciascio G. D., Feng C. F., Feng Z., Gao W., Gou Q. B., Guo Y. Q., He H. H., Hu H., Iacovacci M., Iuppa R., Jia H. Y., Labaciren, Li H. J., Li Z., Liu C., Liu J., Liu M. Y., Lu H., Ma L. L., Ma X. H., Mancarella G., Mari S. M., Marsella G., Mastroianni S., Montini P., Ning C. C., Perrone L., Pistilli P., Salvini P., Santonico R., Shen P. R., Sheng X. D., Shi F., Surdo A., Tan Y. H., Vallania P., Vernetto S., Vigorito C., Wang H., Wu C. Y., Wu H. R., Xue L., Yang Q. Y., Yang X. C., Yao Z. G., Yuan A. F., Zha M., Zhang H. M., Zhang L., Zhang X. Y., Zhang Y., Zhao J., Zhaxiciren Zhaxisangzhu, Zhou X. X., Zhu F. R., Zhu Q. Q., Bartoli, B., Bernardini, P., Bi, X. J., Cao, Z., Catalanotti, S., Chen, S. Z., Chen, T. L., Cui, S. W., Dai, B. Z., D'Amone, A., Mitri, I. D., Piazzoli, B. D., Girolamo, T. D., Sciascio, G. D., Feng, C. F., Feng, Z., Gao, W., Gou, Q. B., Guo, Y. Q., He, H. H., Hu, H., Iacovacci, M., Iuppa, R., Jia, H. Y., Li, H. J., Li, Z., Liu, C., Liu, J., Liu, M. Y., Lu, H., Ma, L. L., Ma, X. H., Mancarella, G., Mari, S. M., Marsella, G., Mastroianni, S., Montini, P., Ning, C. C., Perrone, L., Pistilli, P., Salvini, P., Santonico, R., Shen, P. R., Sheng, X. D., Shi, F., Surdo, A., Tan, Y. H., Vallania, P., Vernetto, S., Vigorito, C., Wang, H., Wu, C. Y., Wu, H. R., Xue, L., Yang, Q. Y., Yang, X. C., Yao, Z. G., Yuan, A. F., Zha, M., Zhang, H. M., Zhang, L., Zhang, X. Y., Zhang, Y., Zhao, J., Zhaxiciren, Zhaxisangzhu, Zhou, X. X., Zhu, F. R., Zhu, Q. Q., D’Amone, A., Danzengluobu, Null, Mitri, I. De, Piazzoli, B. D’Ettorre, Di Girolamo, T., Sciascio, G. Di, Feng, Zhaoyang, Feng, Zhenyong, Hu, Haibing, Hu, Hongbo, Labaciren, Null, Zhaxiciren, Null, and Zhaxisangzhu, Null
Subjects: Solar minimum, Sun: general, Astrophysics::High Energy Astrophysical Phenomena, FOS: Physical sciences, Cosmic ray, astroparticle physics, cosmic rays, gamma rays: general, 7. Clean energy, 01 natural sciences, Atmosphere, 0103 physical sciences, general [Sun], 010303 astronomy & astrophysics, Argo, cosmic ray, High Energy Astrophysical Phenomena (astro-ph.HE), Astroparticle physics, Physics, 010308 nuclear & particles physics, Settore FIS/01 - Fisica Sperimentale, Gamma ray, Astronomy, astroparticle physic, Astronomy and Astrophysics, 13. Climate action, Space and Planetary Science, High Energy Physics::Experiment, Astrophysics::Earth and Planetary Astrophysics, Astrophysics - High Energy Astrophysical Phenomena, general [gamma rays]
Abstract: The hadronic interaction of cosmic rays with solar atmosphere can produce high energy gamma-rays. The gamma-ray luminosity is correlated both with the flux of primary cosmic rays and the intensity of the solar magnetic field. The gamma-rays below 200 GeV have been observed by Fermi without any evident energy cutoff. The bright gamma-ray flux above 100 GeV has been detected only during solar minimum. The only available data in the TeV range come from the HAWC observations, however, outside the solar minimum. The ARGO-YBJ data set has been used to search for sub-TeV/TeV gamma-rays from the Sun during the solar minimum from 2008 to 2010, the same time period covered by the Fermi data. A suitable model containing the Sun shadow, solar disk emission, and inverse-Compton emission has been developed, and the chi-square minimization method was used to quantitatively estimate the disk gamma-ray signal. The result shows that no significant gamma-ray signal is detected and upper limits to the gamma-ray flux at 0.3-7 TeV are set at the 95% confidence level. In the low energy range these limits are consistent with the extrapolation of the Fermi-LAT measurements taken during solar minimum and are compatible with a softening of the gamma-ray spectrum below 1 TeV. They also provide an experimental upper bound to any solar disk emission at TeV energies. Models of dark matter annihilation via long-lived mediators predicting gamma-ray fluxes >10-7 GeV cm-2 s-1 below 1 TeV are ruled out by the ARGO-YBJ limits.
Published: 2019

40. Observation of e+e−→ηY(2175) at center-of-mass energies above 3.7 GeV

Author: D. J. Ambrose, F. E. Maas, T. Hu, X. L. Li, O. Bakina, M. Albrecht, Z. G. Wang, H. Y. Zhang, P. L. Wang, W. D. Li, P. X. Shen, Z. Wu, Z. A. Liu, G. F. Chen, L. W. Jiang, V. Prasad, Y. H. Guan, Y. Ban, P. Weidenkaff, S. Ahmed, F. A. Harris, P. Musiol, Xiaocong Ai, J. Y. Zhang, C. Schnier, Y. Q. Wang, Zhiqing Zhang, S. P. Wen, X. S. Qin, X. R. Zhou, X. T. Huang, G. Rong, Z. P. Zhang, H. Leithoff, Y. X. Yang, E. H. Thorndike, X. H. Liu, L. Q. Qin, Kang Li, S. B. Liu, Y. Nefedov, Y. K. Heng, J. P. Dai, X. C. Chen, X. N. Ma, Cheng Li, S. Q. Zhang, A. Hafner, Q. Zhao, Y. Z. Sun, X. K. Chu, F. De Mori, R. Kliemt, L. H. Wu, H. B. Li, B. Kloss, C. L. Luo, B. Wang, M. Fritsch, M. Savrie, M. M. Ma, C. C. Zhang, H. Liang, B. Zhong, L. B. Guo, Bibo Ke, W. B. Yan, J. Chai, X. Y. Zhou, G. X. Sun, J. V. Bennett, Li Yan, Z. Jiao, D. H. Zhang, M. G. Zhao, Lei Li, Ke Wang, M. Kavatsyuk, F. Li, Jie Yu, R. P. Guo, F. C. Ma, Peilian Liu, Lingxuan Zhang, Gang Zhao, Y. N. Zhang, Y. H. Zheng, S. Pacetti, Cong-Feng Qiao, O. Albayrak, C. Leng, Q. P. Ji, I. Tapan, Y. H. Yan, X. F. Wang, J. W. Zhao, J. M. Bian, R. Poling, S. J. Zhao, B. J. Liu, N. Yu. Muchnoi, T. J. Min, K. J. Zhu, Y. F. Wang, Ke Li, X. S. Kang, T. Ma, Y. H. Zhang, B. X. Zhang, G. Cibinetto, P. F. Duan, F. H. Heinsius, Gianfranco Morello, Jiaxi Liu, Q. M. Ma, Y. C. Zhu, A. A. Zafar, Q. J. Xu, X. Q. Hao, J. F. Qiu, M. Papenbrock, Fenfen An, Xichao Ruan, S. L. Olsen, B. L. Wang, Yang Li, Fang Liu, U. Wiedner, I. Denysenko, Z. Y. Wang, J. C. Chen, Xuanhong Lou, Nasser Kalantar-Nayestanaki, J. Q. Zhang, T. Holtmann, T. C. Zhao, H. R. Qi, L. Fava, C. Morales Morales, Yue Pan, M. H. Gu, F. Nerling, B. Y. Zhang, X. H. Mo, L. S. Wang, M. H. Ye, K. H. Rashid, J. Y. Liu, P. Larin, H. Y. Sheng, C. X. Yu, X. Y. Niu, Y. Yuan, Y. S. Zhu, G. F. Xu, S. Jin, Yu Zhang, J. Z. Bai, H. Xiao, T. Held, A. Calcaterra, Z. G. Zhao, Q. A. Malik, G. Mezzadri, Y. T. Liang, S. J. Chen, Y. P. Guo, Serkant Ali Cetin, B. Zheng, R. G. Ping, R. Baldini Ferroli, L. L. Wang, H. Cai, Huanhuan Liu, M. Y. Dong, T. Hussain, X. Y. Ma, W. X. Gong, Yang Zhang, M. N. Achasov, L. P. Zhou, Y. M. Ma, S. Z. Chen, G. S. Huang, F. Feldbauer, Z. L. Huang, Feng Liu, Q. Gao, Y. N. Gao, Dan Wang, J. H. Zou, S. S. Sun, Q. Liu, Tristan Weber, M. Ablikim, J. B. Jiao, Manuel Lara, Jie Zhao, D. X. Lin, Z. P. Mao, J. Fang, Tao Li, Alexey Zhemchugov, H. M. Hu, Krisztian Peters, M. Z. Wang, F. H. Liu, Nicolas Berger, X. Y. Jiang, X. Y. Song, L. D. Liu, L. L. Ma, G. Felici, H. H. Zhang, J. Z. Fan, J. W. Zhang, X. N. Li, X. P. Xu, X. B. Ji, M. Tiemens, R. E. Mitchell, L. Y. Dong, L. Gong, Ch. Rosner, L. G. Xia, A. Amoroso, J. J. Xu, C. H. Li, X. H. Sun, Haiping Peng, Tao Luo, G. R. Liao, Z. J. Sun, H. Loehner, P. Patteri, Yunlong Zhang, Z. Gao, W. J. Zheng, A. Dbeyssi, Jun-Yi Zhang, J. S. Huang, Yao Wang, M. Kornicer, C. X. Liu, L. Zotti, D. W. Bennett, Zujian Wang, S. L. Niu, B. X. Yu, Zhi Zeng, R. Farinelli, Yao Zhang, D. Bettoni, A. Julin, X. Q. Li, G. Li, Y. B. Zhao, J. F. Sun, Y. F. Long, W. Shan, F. Y. Li, J. Dong, M. Bertani, S. Qian, J. L. Zhang, I. B. Nikolaev, Z. Haddadi, S. Nisar, Q. An, Jialun Ping, C. J. Tang, Y. Hu, Y. P. Lu, K. Goetzen, K. Zhang, H. S. Chen, S. Marcello, H. L. Ma, D. M. Li, Alperen Yuncu, Jin Li, Y. Zeng, Yaquan Fang, M. Greco, D. Xiao, Shou-hua Zhu, C. D. Fu, C. Q. Feng, J. C. Li, X. R. Chen, X. Y. Zhang, L. Yang, Zhe Sun, J. H. Yin, M. Shao, Y. T. Gu, H. L. Dai, Z. Y. Deng, M. Ripka, H. Muramatsu, Y. X. Xia, J. Zhuang, J. B. Liu, Jianping Zheng, M. X. Luo, M. Pelizaeus, Y. B. Chen, Xiaofeng Zhu, J. Z. Zhang, Y. J. Sun, E. Boger, D. V. Dedovich, S. Zhu, X. K. Zhou, E. Fioravanti, K. Schoenning, Q. Y. Li, B. S. Zou, K. Y. Liu, X. L. Kang, A. Sarantsev, D. H. Wei, P. R. Li, J. S. Lange, S. X. Du, Q. W. Zhao, Z. B. Li, W. Ikegami Andersson, H. J. Li, Z. Ning, W. Gradl, J. J. Zhang, M. Destefanis, P. Kiese, D. Y. Wang, C. Hu, X. Tang, Q. L. Xiu, M. Qi, H. J. Yang, R. A. Briere, X. S. Jiang, X. L. Luo, Zhiqing Liu, X. L. Gao, C. Dong, S. Sosio, T. Johansson, J. F. Chang, J. Min, Joachim Pettersson, Y. N. Guo, H. B. Liu, W. P. Wang, O. B. Kolcu, B. Kopf, O. Cakir, K. L. He, X. Cai, F. Bianchi, S. W. Han, Jimin Zhao, C. F. Redmer, D. Y. Liu, W. G. Li, A. G. Denig, S. Spataro, Y. Y. Liu, Zongyuan Wang, H. M. Liu, G. A. Chelkov, G. F. Cao, Y. J. Mao, Xiao-Rui Lyu, Q. Ouyang, H. X. Yang, I. Garzia, G. S. Varner, Y. H. Xie, Huihui Liu, M. Maggiora, Ling Zhao, S. S. Fang, J. P. Liu, J. G. Messchendorp, Lei Zhao, Qiunan Xu, Y. B. Liu, Z. L. Hou, A. Q. Guo, X. L. Ji, W. M. Song, Z. Y. Zhang, C. Z. Yuan, Z. H. Qin, Y. G. Xie, Z. L. Dou, L. J. Wu, Y. J. Mo, I. R. Boyko, Liqing Xu, X. Y. Shen, Y. Ding, W. Kühn, Z. Y. You, Z. A. Zhu, C. P. Shen, I. Uman, Z. J. Xiao, Xiaozhong Huang, Andrzej Kupsc, M. L. Chen, Magnus Wolke, Y. F. Liang, D. P. Jin, N. Qin, H. J. Lu, and J. G. Lu
Subjects: Physics, Nuclear physics, 010308 nuclear & particles physics, Electron–positron annihilation, 0103 physical sciences, Center of mass, 010306 general physics, 01 natural sciences, Storage ring
Abstract: The state Y(2175) is observed in the process e+e-→ηY(2175) with a statistical significance larger than 10 standard deviations using the data collected with the BESIII detector operating at the BEPCII storage ring at center-of-mass energies between 3.7 and 4.6 GeV. This is the first observation of the Y(2175) in this process. The mass and width of the Y(2175) are determined to be (2135±8±9) MeV/c2 and (104±24±12) MeV, respectively, and the production cross section (σ) of e+e-→ηY(2175)→ηϕf0(980)→ηϕπ+π- is at the several hundred femtobarn level. No significant signal for the process e+e-→η′Y(2175) is observed and the upper limit on σ(e+e-→η′Y(2175))/σ(e+e-→ηY(2175)) is estimated to be 0.43 at the 90% confidence level. We also search for ψ(3686)→ηY(2175). No significant signal is observed, indicating a strong suppression relative to the corresponding J/ψ decay, in violation of the “12% rule”.
Published: 2019

41. [Effects of menopausal factor on fine anatomy of bladder urethra and vagina in women undergoing vaginal delivery]

Author: L, Chen, C L, Chen, P, Liu, J, Feng, W W, Qiao, L, Tang, S Z, Chen, J Y, Chen, and X J, Cao
Subjects: Adult, Male, Pregnancy, Urinary Bladder, Vagina, Humans, Female, Menopause, Delivery, Obstetric
Published: 2018

42. Observation of the Crab Nebula with LHAASO-KM2A − a performance study *

Author: F. Aharonian, Q. An, 克古 Axikegu, L. X. Bai, Y. X. Bai, Y. W. Bao, D. Bastieri, X. J. Bi, Y. J. Bi, H. Cai, J. T. Cai, Z. Cao, J. Chang, J. F. Chang, X. C. Chang, B. M. Chen, J. Chen, L. Chen, M. J. Chen, M. L. Chen, Q. H. Chen, S. H. Chen, S. Z. Chen, T. L. Chen, X. L. Chen, Y. Chen, N. Cheng, Y. D. Cheng, S. W. Cui, X. H. Cui, Y. D. Cui, B. Z. Dai, H. L. Dai, Z. G. Dai, 罗布 Danzengluobu, D. della Volpe, B. D'Ettorre Piazzoli, X. J. Dong, J. H. Fan, Y. Z. Fan, Z. X. Fan, J. Fang, K. Fang, C. F. Feng, L. Feng, S. H. Feng, Y. L. Feng, B. Gao, C. D. Gao, Q. Gao, W. Gao, M. M. Ge, L. S. Geng, G. H. Gong, Q. B. Gou, M. H. Gu, J. G. Guo, X. L. Guo, Y. Q. Guo, Y. Y. Guo, Y. A. Han, H. H. He, H. N. He, J. C. He, S. L. He, X. B. He, Y. He, M. Heller, Y. K. Hor, C. Hou, X. Hou, H. B. Hu, S. Hu, S. C. Hu, X. J. Hu, D. H. Huang, Q. L. Huang, W. H. Huang, X. T. Huang, Z. C. Huang, F. Ji, X. L. Ji, H. Y. Jia, K. Jiang, Z. J. Jiang, C. Jin, D. Kuleshov, K. Levochkin, B. B. Li, C. Li, F. Li, H. B. Li, H. C. Li, H. Y. Li, J. Li, K. Li, W. L. Li, X. Li, X. R. Li, Y. Li, Y. Z. Li, Z. Li, E. W. Liang, Y. F. Liang, S. J. Lin, B. Liu, C. Liu, D. Liu, H. Liu, H. D. Liu, J. Liu, J. L. Liu, J. S. Liu, J. Y. Liu, M. Y. Liu, R. Y. Liu, S. M. Liu, W. Liu, Y. N. Liu, Z. X. Liu, W. J. Long, R. Lu, H. K. Lv, B. Q. Ma, L. L. Ma, X. H. Ma, J. R. Mao, A. Masood, W. Mitthumsiri, T. Montaruli, Y. C. Nan, B. Y. Pang, P. Pattarakijwanich, Z. Y. Pei, M. Y. Qi, D. Ruffolo, V. Rulev, A. Sáiz, L. Shao, O. Shchegolev, X. D. Sheng, J. R. Shi, H. C. Song, Yu. V. Stenkin, V. Stepanov, Q. N. Sun, X. N. Sun, Z. B. Sun, P. H. T. Tam, Z. B. Tang, W. W. Tian, B. D. Wang, C. Wang, H. Wang, H. G. Wang, J. C. Wang, J. S. Wang, L. P. Wang, L. Y. Wang, R. N. Wang, W. Wang, X. G. Wang, X. J. Wang, X. Y. Wang, Y. D. Wang, Y. J. Wang, Y. P. Wang, Z. Wang, Z. H. Wang, Z. X. Wang, D. M. Wei, J. J. Wei, Y. J. Wei, T. Wen, C. Y. Wu, H. R. Wu, S. Wu, W. X. Wu, X. F. Wu, S. Q. Xi, J. Xia, J. J. Xia, G. M. Xiang, G. Xiao, H. B. Xiao, G. G. Xin, Y. L. Xin, Y. Xing, D. L. Xu, R. X. Xu, L. Xue, D. H. Yan, C. W. Yang, F. F. Yang, J. Y. Yang, L. L. Yang, M. J. Yang, R. Z. Yang, S. B. Yang, Y. H. Yao, Z. G. Yao, Y. M. Ye, L. Q. Yin, N. Yin, X. H. You, Z. Y. You, Y. H. Yu, Q. Yuan, H. D. Zeng, T. X. Zeng, W. Zeng, Z. K. Zeng, M. Zha, X. X. Zhai, B. B. Zhang, H. M. Zhang, H. Y. Zhang, J. L. Zhang, J. W. Zhang, L. Zhang, L. X. Zhang, P. F. Zhang, P. P. Zhang, R. Zhang, S. R. Zhang, S. S. Zhang, X. Zhang, X. P. Zhang, Y. Zhang, Y. F. Zhang, Y. L. Zhang, B. Zhao, J. Zhao, L. Zhao, L. Z. Zhao, S. P. Zhao, F. Zheng, Y. Zheng, B. Zhou, H. Zhou, J. N. Zhou, P. Zhou, R. Zhou, X. X. Zhou, C. G. Zhu, F. R. Zhu, H. Zhu, K. J. Zhu, and X. Zuo
Subjects: Physics, Nuclear and High Energy Physics, High energy, 010308 nuclear & particles physics, Cosmic distance ladder, Astronomy and Astrophysics, Astrophysics, 01 natural sciences, Crab Nebula, 0103 physical sciences, Energy spectrum, 010306 general physics, Instrumentation, Energy (signal processing)
Abstract: A sub-array of the Large High Altitude Air Shower Observatory (LHAASO), KM2A is mainly designed to observe a large fraction of the northern sky to hunt for γ-ray sources at energies above 10 TeV. Even though the detector construction is still underway, half of the KM2A array has been operating stably since the end of 2019. In this paper, we present the KM2A data analysis pipeline and the first observation of the Crab Nebula, a standard candle in very high energy γ-ray astronomy. We detect γ-ray signals from the Crab Nebula in both energy ranges of 10 100 TeV and 100 TeV with high significance, by analyzing the KM2A data of 136 live days between December 2019 and May 2020. With the observations, we test the detector performance, including angular resolution, pointing accuracy and cosmic-ray background rejection power. The energy spectrum of the Crab Nebula in the energy range 10-250 TeV fits well with a single power-law function dN/dE = (1.13 0.05 0.08 ) 10 (E/20 TeV) cm s TeV . It is consistent with previous measurements by other experiments. This opens a new window of γ-ray astronomy above 0.1 PeV through which new ultrahigh-energy γ-ray phenomena, such as cosmic PeVatrons, might be discovered.
Published: 2021

43. The miR-181d-regulated metalloproteinase Adamts1 enzymatically impairs adipogenesis via ECM remodeling

Author: Wei Jia, Hai Yan Huang, S. Z. Chen, W. Y. Jiang, Xiaoli Chen, Chun Xing, Qi Qun Tang, L. F. Ning, and Xu Xu
Subjects: Adult, 0301 basic medicine, medicine.medical_specialty, Adipose tissue, Bone Morphogenetic Protein 4, Biology, Models, Biological, Extracellular matrix, Young Adult, 03 medical and health sciences, chemistry.chemical_compound, 0302 clinical medicine, Downregulation and upregulation, ADAMTS1 Protein, Internal medicine, Adipocyte, Adipocytes, medicine, Animals, Homeostasis, Humans, Cell Lineage, Obesity, Extracellular Signal-Regulated MAP Kinases, Molecular Biology, Original Paper, Metalloproteinase, Thrombospondin, Adipogenesis, Base Sequence, Organ Size, Cell Biology, Middle Aged, Extracellular Matrix, Cell biology, Mice, Inbred C57BL, MicroRNAs, 030104 developmental biology, Endocrinology, Adipose Tissue, chemistry, 030220 oncology & carcinogenesis, Signal transduction
Abstract: The extracellular matrix (ECM) maintenance is crucial to the structural integrity of adipocytes and whole adipose tissue formation. However, the potential impact of the ECM on adipocyte lineage commitment is unclear. Herein, we demonstrate that forced expression of matrix-associated metalloproteinase Adamts1 (a disintegrin and metalloproteinase with thrombospondin motifs 1), which we show is targeted by microRNA-181d (miR-181d) during BMP4-induced adipocytic lineage commitment, markedly impairs adipocyte commitment. Conversely, siRNA-induced inhibition of Adamts1 promotes adipocyte commitment. Adamst1 metalloprotease activity is required for this inhibition and is determined to function via remodeling ECM components followed by activating FAK-ERK signaling pathway during the commitment process. Furthermore, ablation of Adamts1 in adipose tissue increases adipose tissue mass, reduces insulin sensitivity, and disrupts lipid homeostasis. This finding is consistent with Adamts1 decreased expression in the adipose tissue of obese mice and an inverse correlation of Adamts1 expression with body mass index in humans. Collectively, our results indicate that Adamts1 acts as an ECM 'modifier', with miR-181d-induced downregulation, that regulates adipocyte lineage commitment and obesity.
Published: 2016

44. The ARGO-YBJ experiment in Tibet

Author: THE ARGO YBJ COLLABORATION G. Aielli a, b, C. Bacci c, d, B. Bartoli e, f, P. Bernardini g, h, X. J. Bi i, C. Bleve g, P. Branchini d, A. Budano d, S. Bussino c, A. K. Calabrese Melcarne x, P. Camarri a, Z. Cao i, A. Cappa j, k, R. Cardarelli b, S. Catalanotti f, e, C. Cattaneo l, P. Celio c, S. Z. Chen i, Y. Chen i, N. Cheng i, P. Creti h, S. W. Cuim, B. Z. Dai o, G. D’Alí Staiti n, p, Danzengluobu q, M. Dattoli j, k, r, I. De Mitri g, B. D’Ettorre Piazzoli f, M. De Vincenzi c, T. Di Girolamo f, X. H. Ding q, G. Di Sciascio b, C. F. Feng s, Zhaoyang Feng i, Zhenyong Feng t, F. Galeazzi d, P. Galeotti j, r, R. Gargana d, Q. B. Gou i, Y. Q. Guo i, H. H. He i, Haibing Huq, Hongbo Hui, Q. Huang t, M. Iacovacci f, R. Iuppa a, I. James c, H. Y. Jia t, Labaciren q, H. J. Li q, J. Y. Li s, X. X. Li i, B. Liberti b, G. Liguori l, u, C. Liu i, C. Q. Liu o, M. Y. Lium, J. Liu o, H. Lui, X. H. Mai, G. Mancarella g, c, d, G. Marsella h, v, D. Martello g, S. Mastroianni e, X. R. Meng q, P. Montini c, C. C. Ning q, A. Pagliaro n, w, M. Panareo h, L. Perrone h, P. Pistilli c, X. B. Qu s, E. Rossi e, F. Ruggieri d, L. Saggese f, P. Salvini l, R. Santonico a, P. R. Shen i, X. D. Sheng i, F. Shi i, C. Stanescu d, A. Surdo h, Y. H. Tan i, P. Vallania j, S. Vernetto j, C. Vigorito j, B. Wangi, H. Wang i, C. Y. Wui, H. R. Wui, B. Xut, L. Xues, Y. X. Yanm, Q. Y. Yang o, X. C. Yang o, A. F. Yuan q, M. Zha i, H. M. Zhang i, JiLong Zhang i, JianLi Zhang i, L. Zhang o, P. Zhang o, X. Y. Zhang s, Y. Zhang i, Zhaxisangzhu q, X. X. Zhou t, F. R. Zhu i, Q. Q. Zhu i, G. Zizzi g, MARI, Stefano Maria, D'ALI' STAITI G, Aielli, G, Bacci, C, Bartoli, B, Bernardini, P, Bi, Xj, Bleve, C, Branchini, P, Budano, A, Bussino, Severino Angelo Maria, Calabrese Melcarne, Ak, Camarri, P, Cao, Z, Cappa, A, Cardarelli, R, Catalanotti, S, Cattaneo, C, Celio, P, Chen, Sz, Chen, Tl, Chen, Y, Cheng, N, Creti, P, Cui, Sw, Dai, Bz, D'Ali Staiti, G, Danzengluobu, Dattoli, M, De Mitri, I, D'Ettorre Piazzoli, B, De Vincenzi, M, Di Girolamo, T, Ding, Xh, Di Sciascio, G, Feng, Cf, Feng Zhao, Yang, Feng Zhen, Yong, Galeazzi, F, Galeotti, P, Gargana, R, Gou, Qb, Guo, Yq, He, Hh, Hu, Haibing, Hu Hong, Bo, Huang, Q, Iacovacci, M, Iuppa, R, James, I, Jia, Hy, Labaciren, Li, Hj, Li, Jy, Li, Xx, Liberti, B, Liguori, G, Liu, C, Liu, Cq, Liu, My, Liu, J, Lu, H, Ma, Xh, Mancarella, G, Mari, Stefano Maria, Marsella, G, Martello, D, Mastroianni, S, Meng, Xr, Montini, P, Ning, Cc, Pagliaro, A, Panareo, M, Perrone, L, Pistilli, P, Qu, Xb, Rossi, E, Ruggieri, F, Saggese, L, Salvini, P, Santonico, R, Shen, Pr, Sheng, Xd, Shi, F, Stanescu, C, Surdo, A, Tan, Yh, Vallania, P, Vernetto, S, Vigorito, C, Wang, B, Wang, H, Wu, Cy, Wu, Hr, Xu, B, Xue, L, Yan, Yx, Yang, Qy, Yang, Xc, Yuan, Af, Zha, M, Zhang, Hm, Zhang Ji, Long, Zhang Jian, Li, Zhang, L, Zhang, P, Zhang, Xy, Zhang, Y, Zhaxisangzhu, Zhou, Xx, Zhu, Fr, Zhu, Qq, Zizzi, G., G., Aielli, C., Bacci, F., Barone, B., Bartoli, Bernardini, Paolo, X. J., Bi, C., Bleve, P., Branchini, A., Budano, S., Bussino, A. K., Calabrese Melcarne, P., Camarri, Z., Cao, A., Cappa, R., Cardarelli, S., Catalanotti, C., Cattaneo, S., Cavaliere, P., Celio, S. Z., Chen, N., Cheng, P., Creti, S. W., Cui, G., Cusumano, B. Z., Dai, G., D’Alí Staiti, M., Dattoli, DE MITRI, Ivan, R., De Rosa, B., D’Ettorre Piazzoli, M., De Vincenzi, T., Di Girolamo, X. H., Ding, G., Di Sciascio, C. F., Feng, Zhaoyang, Feng, Zhenyong, Feng, C., Ferrigno, F., Galeazzi, P., Galeotti, X. Y., Gao, R., Gargana, F., Garufi, Q. B., Gou, H. H., He, Haibing, Hu, Hongbo, Hu, Q., Huang, M., Iacovacci, I., Jame, H. Y., Jia, H. J., Li, J. Y., Li, B., Liberti, G., Liguori, C. Q., Liu, J., Liu, H., Lu, Mancarella, Giovanni, S. M., Mari, Marsella, Giovanni, Martello, Daniele, S., Mastroianni, X. R., Meng, J., Mu, L., Nicastro, C. C., Ning, L., Palummo, Panareo, Marco, Perrone, Lorenzo, P., Pistilli, X. B., Qu, E., Rossi, F., Ruggieri, L., Saggese, P., Salvini, R., Santonico, A., Segreto, P. R., Shen, X. D., Sheng, F., Shi, C., Stanescu, A., Surdo, Y. H., Tan, P., Vallania, S., Vernetto, C., Vigorito, H., Wang, Y. G., Wang, C. Y., Wu, H. R., Wu, B., Xu, L., Xue, H. T., Yang, Q. Y., Yang, X. C., Yang, G. C., Yu, A. F., Yuan, M., Zha, H. M., Zhang, J. L., Zhang, L., Zhang, P., Zhang, X. Y., Zhang, Y., Zhang, X. X., Zhou, F. R., Zhu, Q. Q., Zhu, G., Zizzi, THE ARGO YBJ COLLABORATION G., Aielli a, B, C., Bacci c, D, B., Bartoli e, F, P., Bernardini g, H, X. J., Bi i, C., Bleve g, P., Branchini d, A., Budano d, S., Bussino c, A. K., Calabrese Melcarne x, P., Camarri a, Z., Cao i, A., Cappa j, K, R., Cardarelli b, S., Catalanotti f, E, C., Cattaneo l, P., Celio c, S. Z., Chen i, Y., Chen i, N., Cheng i, P., Creti h, S. W., Cuim, B. Z., Dai o, G., D’Alí Staiti n, P, Danzengluobu, Q, M., Dattoli j, K, R, I., De Mitri g, B., D’Ettorre Piazzoli f, M., De Vincenzi c, T., Di Girolamo f, X. H., Ding q, G., Di Sciascio b, Zhaoyang Feng, I, Zhenyong Feng, T, F., Galeazzi d, P., Galeotti j, R, R., Gargana d, Q. B., Gou i, Y. Q., Guo i, H. H., He i, Haibing, Huq, Hongbo, Hui, Q., Huang t, M., Iacovacci f, R., Iuppa a, I., James c, H. Y., Jia t, Labaciren, Q, H. J., Li q, X. X., Li i, B., Liberti b, G., Liguori l, U, C., Liu i, C. Q., Liu o, M. Y., Lium, J., Liu o, H., Lui, X. H., Mai, G., Mancarella g, C, D, G., Marsella h, V, D., Martello g, S., Mastroianni e, X. R., Meng q, P., Montini c, C. C., Ning q, A., Pagliaro n, W, M., Panareo h, L., Perrone h, P., Pistilli c, E., Rossi e, F., Ruggieri d, L., Saggese f, P., Salvini l, R., Santonico a, P. R., Shen i, X. D., Sheng i, F., Shi i, C., Stanescu d, A., Surdo h, Y. H., Tan i, P., Vallania j, S., Vernetto j, C., Vigorito j, B., Wangi, H., Wang i, C. Y., Wui, H. R., Wui, B., Xut, Y. X., Yanm, Q. Y., Yang o, X. C., Yang o, A. F., Yuan q, M., Zha i, H. M., Zhang i, JiLong Zhang, I, JianLi Zhang, I, L., Zhang o, P., Zhang o, Y., Zhang i, Zhaxisangzhu, Q, X. X., Zhou t, F. R., Zhu i, Q. Q., Zhu i, and G., Zizzi g
Subjects: Physics, Nuclear and High Energy Physics, Gamma ray burst, Single cluster, Trigger rate, Detector, gamma ray bursts, gamma rays, cosmic rays, extended air showers, Astronomy, Sampling (statistics), Cosmic ray, Extended air showers, Cosmic rays, Gamma ray sources, Gamma ray bursts, Gamma ray sources, Geodesy, Guard ring, Extended air shower, Sampling density, Instrumentation, Argo
Abstract: The setting up of the ARGO detector at the YangBaJing Cosmic Ray Laboratory (4300 m a.s.l., Tibet, P.R. China) has been completed during the last spring (2007). It consists of a central carpet made of 130 identical sub-units of 12 RPCs each (a "cluster"), covering a surface of about 5800 m2 with 93% active area, and a guard ring of 24 further clusters of the same type surrounding the central carpet with a lower sampling density. Signals are picked up by external electrodes of small size, thus allowing the sampling of EAS with high space-time granularity. Shower events are detected at a trigger rate of about 4 kHz. Events with a few particles detected by a single cluster are counted in scaler mode on a time base of 500 ms. The intrinsic modularity of the ARGO detector allowed us to collect data even during the setting-up period, using only the central carpet (or even part of it). Some preliminary results from the analysis of events collected in a few months of data taking are presented. © 2008 Elsevier B.V. All rights reserved.
Published: 2008

45. The analog Resistive Plate Chamber detector of the ARGO-YBJ experiment

Author: Zihuang Cao, M. Iacovacci, M. Zha, J. W. Zhao, P. Pistilli, H. M. Zhang, Paolo Camarri, X. X. Zhou, J. K. K. Liu, X. Y. Zhang, P. Creti, Haibing Hu, Minghui Liu, Hongbo Hu, Haifeng Li, A. Surdo, Y. Zhang, D. Martello, Lanqing Ma, Yicheng Guo, Danzengluobu, Carlo Vigorito, S. W. Cui, P. Montini, X. H. Ma, Q. Q. Zhu, G. Di Sciascio, H. W. Wang, Zhaxisangzhu, A. Budano, H. Y. Jia, Fudong Shi, Labaciren, S. Mastroianni, Zhaxiciren, T. Di Girolamo, A. F. Yuan, G. Liguori, C. X. Liu, H. R. Wu, B. Z. Dai, F. Ruggieri, Q. Y. Yang, G. Zizzi, P. Branchini, R. Santonico, A. D'Amone, F. R. Zhu, S. Vernetto, H. Lu, R. Cardarelli, G. Marsella, L. Perrone, L. Zhang, P. Salvini, Cunfeng Feng, P. Bernardini, Y. H. Tan, Z. G. Yao, X. D. Sheng, Giovanni Mancarella, H. H. He, X. C. Yang, Chang-Chun Ning, Zhaoyang Feng, M. Panareo, P. Vallania, B. D'Ettorre Piazzoli, I. De Mitri, C. Y. Wu, L. Xue, Q. B. Gou, T. L. Chen, Zhenyong Feng, X. J. Bi, S. Z. Chen, B. Bartoli, S. M. Mari, Pengnian Shen, S. Catalanotti, R. Iuppa, ITA, Bartoli, Bruno, Bernardini, P., Bi, X. J., Branchini, P., Budano, A., Camarri, P., Cao, Z., Cardarelli, R., Catalanotti, Sergio, Chen, S. Z., Chen, T. L., Creti, P., Cui, S. W., Dai, B. Z., D’Amone, A., Danzengluobu, Null, De Mitri, I., D'ETTORRE PIAZZOLI, Benedetto, DI GIROLAMO, Tristano, Di Sciascio, G., Feng, C. F., Feng, Zhaoyang, Feng, Zhenyong, Gou, Q. B., Guo, Y. Q., He, H. H., Hu, Haibing, Hu, Hongbo, Iacovacci, Michele, Iuppa, R., Jia, H. Y., Labaciren, Null, Li, H. J., Liguori, G., Liu, C., Liu, J., Liu, M. Y., Lu, H., Ma, L. L., Ma, X. H., Mancarella, G., Mari, S. M., Marsella, G., Martello, D., Mastroianni, S., Montini, P., Ning, C. C., Panareo, M., Perrone, L., Pistilli, P., Ruggieri, F., Salvini, P., Santonico, R., Shen, P. R., Sheng, X. D., Shi, F., Surdo, A., Tan, Y. H., Vallania, P., Vernetto, S., Vigorito, C., Wang, H., Wu, C. Y., Wu, H. R., Xue, L., Yang, Q. Y., Yang, X. C., Yao, Z. G., Yuan, A. F., Zha, M., Zhang, H. M., Zhang, L., Zhang, X. Y., Zhang, Y., Zhao, J., Zhaxiciren, Null, Zhaxisangzhu, Null, Zhou, X. X., Zhu, F. R., Zhu, Q. Q., Zizzi, G., B. Bartoli, BERNARDINI, Paolo, X. J. Bi, P. Branchini, A. Budano, P. Camarri, Z. Cao, R. Cardarelli, S. Catalanotti, S. Z. Chen, T. L. Chen, P. Creti, S. W. Cui, B. Z. Dai, D'AMONE, ANTONIO, Danzengluobu, DE MITRI, Ivan, B. D’Ettorre Piazzoli, T. Di Girolamo, G. Di Sciascio, C. F. Feng, Zhaoyang Feng, Zhenyong Feng, Q. B. Gou, Y. Q. Guo, H. H. He, Haibing Hu, Hongbo Hu, M. Iacovacci, R. Iuppa, H. Y. Jia, Labaciren, H. J. Li, G. Liguori, C. Liu, J. Liu, M. Y. Liu, H. Lu, L. L. Ma, X. H. Ma, MANCARELLA, Giovanni, S. M. Mari, MARSELLA, GIOVANNI, MARTELLO, Daniele, S. Mastroianni, P. Montini, C. C. Ning, PANAREO, Marco, PERRONE, Lorenzo, P. Pistilli, F. Ruggieri, P. Salvini, R. Santonico, P. R. Shen, X. D. Sheng, F. Shi, A. Surdo, Y. H. Tan, P. Vallania, S. Vernetto, C. Vigorito, H. Wang, C. Y. Wu, H. R. Wu, L. Xue, Q. Y. Yang, X. C. Yang, Z. G. Yao, A. F. Yuan, M. Zha, H. M. Zhang, L. Zhang, X. Y. Zhang, Y. Zhang, J. Zhao, Zhaxiciren, Zhaxisangzhu, X. X. Zhou, F. R. Zhu, Q. Q. Zhu, G. Zizzi, B., Bartoli, Bernardini, Paolo, X. J., Bi, P., Branchini, A., Budano, P., Camarri, Z., Cao, R., Cardarelli, S., Catalanotti, S. Z., Chen, T. L., Chen, P., Creti, S. W., Cui, B. Z., Dai, D'Amone, Antonio, B., D’Ettorre Piazzoli, T., Di Girolamo, G., Di Sciascio, C. F., Feng, Zhaoyang, Feng, Zhenyong, Feng, Q. B., Gou, Y. Q., Guo, H. H., He, Haibing, Hu, Hongbo, Hu, M., Iacovacci, R., Iuppa, H. Y., Jia, H. J., Li, G., Liguori, C., Liu, J., Liu, M. Y., Liu, H., Lu, L. L., Ma, X. H., Ma, Mancarella, Giovanni, S. M., Mari, Marsella, Giovanni, Martello, Daniele, S., Mastroianni, P., Montini, C. C., Ning, Panareo, Marco, Perrone, Lorenzo, P., Pistilli, F., Ruggieri, P., Salvini, R., Santonico, P. R., Shen, X. D., Sheng, F., Shi, A., Surdo, Y. H., Tan, P., Vallania, S., Vernetto, C., Vigorito, H., Wang, C. Y., Wu, H. R., Wu, L., Xue, Q. Y., Yang, X. C., Yang, Z. G., Yao, A. F., Yuan, M., Zha, H. M., Zhang, L., Zhang, X. Y., Zhang, Y., Zhang, J., Zhao, X. X., Zhou, F. R., Zhu, Q. Q., Zhu, G., Zizzi, Mari, Stefano Maria, and The ARGO YBJ, Collaboration
Subjects: Physics - Instrumentation and Detectors, Physics::Instrumentation and Detectors, Astrophysics::High Energy Astrophysical Phenomena, Air shower detection, FOS: Physical sciences, Cosmic ray, STRIPS, Calorimetry, Signal, law.invention, Optics, Observatory, law, Air shower detection, RPC detector, Calorimetry, Cosmic-ray observatory, physics.ins-det, Instrumentation and Methods for Astrophysics (astro-ph.IM), Physics, Resistive touchscreen, business.industry, Detector, Settore FIS/01 - Fisica Sperimentale, Astrophysics::Instrumentation and Methods for Astrophysics, Astronomy and Astrophysics, Instrumentation and Detectors (physics.ins-det), Core (optical fiber), RPC detector, business, Astrophysics - Instrumentation and Methods for Astrophysics, astro-ph.IM
Abstract: The ARGO-YBJ experiment has been in stable data taking from November 2007 till February 2013 at the YangBaJing Cosmic Ray Observatory (4300 m a.s.l.). The detector consists of a single layer of Resistive Plate Chambers (RPCs) (6700 m2) operated in streamer mode. The signal pick-up is obtained by means of strips facing one side of the gas volume. The digital readout of the signals, while allows a high space–time resolution in the shower front reconstruction, limits the measurable energy to a few hundred TeV. In order to fully investigate the 1–10 PeV region, an analog readout has been implemented by instrumenting each RPC with two large size electrodes facing the other side of the gas volume. Since December 2009 the RPC charge readout has been in operation on the entire central carpet (∼5800 m2). In this configuration the detector is able to measure the particle density at the core position where it ranges from tens to many thousands of particles per m2. Thus ARGO-YBJ provides a highly detailed image of the charge component at the core of air showers. In this paper we describe the analog readout of RPCs in ARGO-YBJ and discuss both the performance of the system and the physical impact on the EAS measurements. The ARGO-YBJ experiment has been in stable data taking from November 2007 till February 2013 at the YangBaJing Cosmic Ray Observatory (4300 m a.s.l.). The detector consists of a single layer of Resistive Plate Chambers (RPCs) (6700 m2) operated in streamer mode. The signal pick-up is obtained by means of strips facing one side of the gas volume. The digital readout of the signals, while allows a high space-time resolution in the shower front reconstruction, limits the measurable energy to a few hundred TeV. In order to fully investigate the 1-10 PeV region, an analog readout has been implemented by instrumenting each RPC with two large size electrodes facing the other side of the gas volume. Since December 2009 the RPC charge readout has been in operation on the entire central carpet (â¼5800 m2). In this configuration the detector is able to measure the particle density at the core position where it ranges from tens to many thousands of particles per m2. Thus ARGO-YBJ provides a highly detailed image of the charge component at the core of air showers. In this paper we describe the analog readout of RPCs in ARGO-YBJ and discuss both the performance of the system and the physical impact on the EAS measurements.
Published: 2015

46. Measurement of muonic and electromagnetic components in cosmic ray air showers using LHAASO-KM2A prototype array

Author: Cong Li, Yuncheng Nan, Jinfan Chang, Hongkui Lv, Hongming Li, Guanghua Gong, S. Z. Chen, Zhe Li, Xiong Zuo, Wei Wang, Huihai He, G. C. Xiao, Hui Wang, Xiurong Li, Minghao Gu, N. Cheng, Wei Gao, Yi Zhang, L. P. Wang, Mohsin Saeed, S. H. Feng, Jia Liu, Xiangdong Sheng, Sha Wu, S. R. Zhang, and Fei Li
Subjects: Physics, Nuclear physics, 010308 nuclear & particles physics, 0103 physical sciences, Cosmic ray, 010306 general physics, 01 natural sciences
Published: 2018

47. Precision Study of η′→γπ+π− Decay Dynamics

Author: X. L. Luo, W. P. Wang, T. Holtmann, G. Felici, L. J. Wu, H. J. Li, Q. L. Xiu, M. Y. Dong, Q. Ouyang, S. L. Niu, S. S. Fang, F. Bianchi, Y. B. Liu, F. Y. Li, Jin Li, X. L. Gao, X. N. Ma, Y. H. Guan, J. Y. Liu, R. Kliemt, M. Tiemens, H. B. Liu, C. Leng, J. F. Sun, Xiao-Rui Lyu, M. H. Gu, X. Q. Li, Y. F. Long, M. Greco, Kai Liu, Y. J. Mo, H. Y. Sheng, M. Maggiora, J. P. Dai, Ling Zhao, J. H. Liu, A. Dbeyssi, Ke Wang, C. Dong, M. H. Ye, S. Marcello, Y. Zeng, F. De Mori, X. Y. Jiang, S. Sosio, Yaquan Fang, Z. G. Zhao, S. Fegan, A. Zallo, J. H. Zou, C. X. Yu, Y. Nefedov, M. M. Ma, J. C. Chen, Lei Zhao, Jie Yu, G. S. Varner, Q. Gao, Y. N. Gao, Joachim Pettersson, Z. L. Hou, X. Cai, Y. Zhang, H. H. Zhang, Y. Ban, X. Y. Zhou, L. Yang, M. Fritsch, B. Zheng, Zahra Haddadi, R. G. Ping, M. G. Zhao, R. P. Guo, H. S. Chen, K. Y. Liu, C. Hu, T. Weber, P. F. Duan, J. Q. Zhang, L. D. Liu, J. Z. Zhang, X. Tang, Z. T. Sun, S. S. Sun, Z. J. Sun, R. Poling, Y. N. Zhang, Guo-Ming Chen, J. Z. Fan, A. Yuncu, M. Kavatsyuk, H. Loehner, X. L. Ji, Z. A. Liu, Cui Li, Y. Pan, L. Y. Dong, Orhan Cakir, B. L. Wang, J. Chai, M. N. Achasov, Q. P. Ji, T. J. Min, K. J. Zhu, K. Schoenning, Q. Y. Li, B. S. Zou, P. Kiese, G. X. Sun, C. Z. Yuan, Z. G. Wang, Niklaus Berger, S. L. Olsen, T. C. Zhao, H. J. Lu, J. G. Lu, V. Prasad, Xianglei Zhu, P. Weidenkaff, F. H. Heinsius, F. Li, X. S. Jiang, F. C. Ma, S. Ahmed, Z. Jiao, Fu-Hu Liu, D. H. Zhang, Liqing Xu, X. Y. Shen, H. Liang, F. E. Maas, T. Hu, R. E. Mitchell, B. X. Zhang, O. Fedorov, W. J. Zheng, Yanwei Wang, Y. X. Yang, Y. G. Xie, X. F. Wang, S. P. Wen, X. S. Qin, W. Gradl, M. Ripka, S. X. Du, X. R. Zhou, Y. Ding, K. Li, Z. L. Dou, Cheng Li, X. K. Zhou, Fang Liu, Krisztian Peters, D. Y. Wang, Guangshun Huang, B. J. Liu, L. Yan, J. C. Li, I. Denysenko, Jun-Yi Zhang, Q. M. Ma, D. Bettoni, Y. P. Guo, S. Schumann, J. Min, I. B. Nikolaev, J. Zhuang, R. Baldini Ferroli, B. Kloss, B. Y. Zhang, J. F. Qiu, W. Kühn, Z. P. Zhang, A. Hafner, Q. Zhao, Dmitri Dedovich, Y. Z. Sun, J. H. Yin, Yao Wang, X. B. Ji, Yunlong Zhang, Q. A. Malik, G. Mezzadri, A. Denig, W. C. Yan, X. Y. Niu, M. X. Luo, Yucheng Huang, M. Shao, Y. T. Gu, Y. F. Wang, L. Fava, B. Kopf, M. Albrecht, Z. Y. You, P. Patteri, Z. A. Zhu, Y. Yuan, Y. S. Zhu, M. Bertani, Yu Zhang, Peilian Liu, F. Nerling, G. R. Liao, J. V. Bennett, P. X. Shen, K. L. He, Xiang Zhou, Zhuoming Li, D. W. Bennett, Zujian Wang, L. P. Zhou, E. Fioravanti, Bibo Ke, J. L. Zhang, J. F. Hu, Zhiyong Zhang, D. J. Ambrose, Z. Wu, W. B. Yan, Y. M. Ma, M. Z. Wang, T. Hussain, X. Y. Ma, X. L. Kang, L. W. Jiang, Z. P. Mao, A. Sarantsev, D. H. Wei, P. R. Li, S. Pacetti, Jimin Zhao, Y. X. Xia, S. H. Zhu, Q. Liu, J. S. Lange, Q. W. Zhao, W. X. Gong, Gueorgui Chelkov, Bingxuan Liu, Jianping Zheng, M. L. Chen, H. P. Cheng, Gang Zhao, X. N. Li, G. Li, X. Fang, S. Zhu, J. Fang, Tao Li, Z. Gao, X. D. Ruan, W. G. Li, M. Qi, Zhiqing Zhang, H. J. Yang, M. Ablikim, Haiping Peng, Z. L. Huang, Feng Liu, L. L. Ma, L. Gong, Y. B. Zhao, Lei Zhang, H. B. Li, C. L. Luo, Ch. Rosner, C. D. Fu, W. Shan, X. H. Sun, J. Dong, P. L. Wang, W. D. Li, Tao Luo, X. H. Mo, L. S. Wang, L. G. Xia, S. Spataro, X. P. Xu, C. Q. Feng, X. R. Chen, Y. Y. Liu, Y. Q. Wang, S. Nisar, C. C. Zhang, B. X. Yu, B. Zhong, L. B. Guo, L. L. Wang, R. Farinelli, Lei Li, C. J. Tang, J. J. Zhang, M. Destefanis, Y. Hu, F. A. Harris, Chi Zhang, H. M. Liu, S. B. Liu, Y. P. Lu, Zhi Zeng, H. Cai, L. Zotti, H. Muramatsu, I. Tapan, Y. H. Yan, H. L. Ma, Ulrich Wiedner, D. M. Li, B. Wang, J. W. Zhao, M. Kornicer, Y. C. Zhu, H. Leithoff, T. Ma, G. Cibinetto, D. Xiao, Y. J. Mao, H. R. Qi, R. A. Briere, H. X. Yang, A. Julin, Z. Y. Deng, Xingguo Li, Z. Ning, H. Xiao, E. Boger, M. Pelizaeus, Igor Boyko, I. Garzia, H. L. Dai, T. Held, Huihui Liu, Serkant Ali Cetin, J. P. Liu, Zhiqing Liu, J. G. Messchendorp, Jie Zhao, D. X. Lin, T. Johansson, Qiunan Xu, M. Shi, S. Qian, O. B. Kolcu, A. Calcaterra, Jialun Ping, A. Amoroso, K. Zhang, A. Q. Guo, X. Y. Zhang, W. M. Song, X. Q. Hao, M. Lara, J. B. Liu, Alexey Zhemchugov, H. M. Hu, Y. J. Sun, Xuesong Liu, Z. H. Qin, D. Y. Liu, J. B. Jiao, S. Q. Zhang, Q An, J. W. Zhang, H. Y. Zhang, I. Uman, P. Larin, S. Z. Chen, J. J. Xu, Y. B. Li, J. S. Huang, C. X. Liu, E. H. Thorndike, L. Q. Qin, J. Z. Bai, F. Feldbauer, X. C. Chen, G. F. Xu, S. Jin, Y. H. Zheng, Cong-Feng Qiao, O. Albayrak, N. Yu. Muchnoi, G. F. Cao, X. S. Kang, Y. H. Zhang, Y. Guo, Z. Y. Wang, Yi Chen, X. K. Chu, X. Y. Song, K. Goetzen, J. Y. Zhang, C. P. Shen, Y. K. Heng, J. M. Bian, S. J. Zhao, Q. J. Xu, Xuanhong Lou, Nasser Kalantar-Nayestanaki, C. Morales Morales, Z. J. Xiao, Z. H. Wang, F. F. An, P. Musiol, C. F. Redmer, Xiaocong Ai, Xiaozhong Huang, C. Schnier, X. T. Huang, G. Rong, Andrzej Kupsc, W. L. Yuan, A. A. Zafar, K. H. Rashid, J. F. Chang, Magnus Wolke, Y. T. Liang, Y. F. Liang, S. J. Chen, D. P. Jin, S. Han, Dayong Wang, N. Qin, L. H. Wu, M. Savrie, and L. Xia
Subjects: Physics, Rho meson, 010308 nuclear & particles physics, Electron–positron annihilation, Background data, Form factor (quantum field theory), General Physics and Astronomy, Resonance, 01 natural sciences, Amplitude, Orders of magnitude (time), 0103 physical sciences, Anomaly (physics), Atomic physics, 010306 general physics
Abstract: Using a low background data sample of 9.7×10^{5} J/ψ→γη^{'}, η^{'}→γπ^{+}π^{-} events, which are 2 orders of magnitude larger than those from the previous experiments, recorded with the BESIII detector at BEPCII, the decay dynamics of η^{'}→γπ^{+}π^{-} are studied with both model-dependent and model-independent approaches. The contributions of ω and the ρ(770)-ω interference are observed for the first time in the decays η^{'}→γπ^{+}π^{-} in both approaches. Additionally, a contribution from the box anomaly or the ρ(1450) resonance is required in the model-dependent approach, while the process specific part of the decay amplitude is determined in the model-independent approach.
Published: 2018

48. Galactic Cosmic-Ray Anisotropy in the Northern hemisphere from the ARGO-YBJ Experiment during 2008-2012

Author: J. Zhao, Hongbo Hu, P. R. Shen, X. C. Yang, A. Surdo, Yicheng Guo, Y. H. Tan, Zhaoyang Feng, F. R. Zhu, X. J. Bi, T. Di Girolamo, J. K. K. Liu, S. Vernetto, Zhaxisangzhu, Zhengguo Cao, S. Z. Chen, Q. Q. Zhu, L. Zhang, T. L. Chen, R. Santonico, S. Mastroianni, C. Vigorito, C. Y. Wu, S. W. Cui, C. Q. Liu, Q. B. Gou, C. C. Ning, P. Vallania, F. Shi, S. M. Mari, B. D'Ettorre Piazzoli, A. D'Amone, H. J. Li, H. R. Wu, Zhaxiciren, R. Iuppa, L. Xue, P. Salvini, G. Marsella, W. Gao, P. Bernardini, H. Wang, H. Lu, Danzengluobu, S. Catalanotti, David Ruffolo, A. F. Yuan, B. Z. Dai, Y. J. Zhang, Huihai He, M. Zha, G. Di Sciascio, X. Y. Zhang, Labaciren, Xiangdong Sheng, P. Pistilli, H. M. Zhang, Minghui Liu, I. De Mitri, Q. Y. Yang, P. Montini, X. H. Ma, X. X. Zhou, L. Perrone, Haibing Hu, L. L. Ma, H. Y. Jia, G. Mancarella, B. Bartoli, Cunfeng Feng, M. Iacovacci, Z. G. Yao, Bartoli, B., Bernardini, P., Bi, X. J., Cao, Z., Catalanotti, S., Chen, S. Z., Chen, T. L., Cui, S. W., Dai, B. Z., D’Amone, A., Danzengluobu, Null, De Mitri, I., Piazzoli, B. D’Ettorre, Di Girolamo, T., Di Sciascio, G., Feng, C. F., Feng, Z. Y., Gao, W., Gou, Q. B., Guo, Y. Q., He, H. H., Hu, Haibing, Hu, Hongbo, Iacovacci, M., Iuppa, R., Jia, H. Y., Labaciren, Null, Li, H. J., Liu, C., Liu, J., Liu, M. Y., Lu, H., Ma, L. L., Ma, X. H., Mancarella, G., Mari, S. M., Marsella, G., Mastroianni, S., Montini, P., Ning, C. C., Perrone, L., Pistilli, P., Ruffolo, D., Salvini, P., Santonico, R., Shen, P. R., Sheng, X. D., Shi, F., Surdo, A., Tan, Y. H., Vallania, P., Vernetto, S., Vigorito, C., Wang, H., Wu, C. Y., Wu, H. R., Xue, L., Yang, Q. Y., Yang, X. C., Yao, Z. G., Yuan, A. F., Zha, M., Zhang, H. M., Zhang, L., Zhang, X. Y., Zhang, Y., Zhao, J., Zhaxiciren, Null, Zhaxisangzhu, Null, Zhou, X. X., Zhu, F. R., Zhu, Q. Q., D'Amone, A., Piazzoli, B. D'Ettorre, Mastroianni, Stefano, Danzengluobu, null, Labaciren, null, Zhaxiciren, null, and Zhaxisangzhu, null
Subjects: Astrophysics::High Energy Astrophysical Phenomena, FOS: Physical sciences, Cosmic ray, 01 natural sciences, cosmic rays, 0103 physical sciences, Anisotropy, 010303 astronomy & astrophysics, Argo, cosmic ray, Astroparticle physics, Physics, High Energy Astrophysical Phenomena (astro-ph.HE), 010308 nuclear & particles physics, Settore FIS/01 - Fisica Sperimentale, Northern Hemisphere, Astronomy, astroparticle physic, Astronomy and Astrophysics, astroparticle physics, cosmic ray anysotropy, argo-ybj, Astronomy and Astrophysic, astroparticle physics, Space and Planetary Science, 13. Climate action, Astrophysics - High Energy Astrophysical Phenomena
Abstract: This paper reports on the observation of the sidereal large-scale anisotropy of cosmic rays using data collected by the ARGO-YBJ experiment over 5 years (2008-2012). This analysis extends previous work limited to the period from 2008 January to 2009 December, near the minimum of solar activity between cycles 23 and 24. With the new data sample, the period of solar cycle 24 from near minimum to maximum is investigated. A new method is used to improve the energy reconstruction, allowing us to cover a much wider energy range, from 4 to 520 TeV. Below 100 TeV, the anisotropy is dominated by two wide regions, the so-called “tail-in” and “loss-cone” features. At higher energies, a dramatic change of the morphology is confirmed. The yearly time dependence of the anisotropy is investigated. Finally, no noticeable variation of cosmic-ray anisotropy with solar activity is observed for a median energy of 7 TeV.
Published: 2018
Full Text: View/download PDF

49. [Distribution and drug resistance of pathogens of blood stream infection in patients with hematological malignancies after chemotherapy]

Author: S Z, Chen, K N, Lin, M, Xiao, X F, Luo, Q, Li, J H, Ren, R Y, Huang, M M, Chen, Z Z, Ally, T, Chen, J D, Yang, and Jianda, Hu
Subjects: 论著, Hematological malignancies, 抗药性, Blood stream infection, Hematologic Neoplasms, Drug Resistance, Bacterial, 恶性血液病, Drug Resistance, Humans, 血流感染, Bacteremia, Microbial Sensitivity Tests, Anti-Bacterial Agents
Abstract: 目的分析福建医科大学附属协和医院血液科血培养的病原菌分布及药敏情况，以了解临床真实世界血流感染状况，为临床合理使用抗菌药物提供依据。方法收集2013年1月至2016年12月福建医科大学附属协和医院血液科临床送检血培养阳性标本分离出的657株病原菌资料并对患者临床资料进行分析。结果 657株血培养阳性菌株中，革兰阴性菌（G−菌）410株（62.4%），革兰阳性菌（G+菌）163株（24.8%），真菌50株（7.6%）。前五位的致病细菌分别为肺炎克雷伯菌（17.5%）、大肠埃希菌（17.2%）、凝固酶阴性葡萄球菌（CNS）（14.9%），铜绿假单胞菌（14.2%）及金黄色葡萄球菌（3.5%）。G−菌中肺炎克雷伯菌和大肠埃希菌产超广谱β内酰胺酶（ESBL）菌株的检出率分别为25.2%和55.8%，产ESBL菌株对抗菌药物的耐药率大多高于非产ESBL菌株。肠杆菌科细菌对碳青霉烯类抗生素、哌拉西林/他唑巴坦、替加环素的耐药率均在14%以下。非发酵菌中，铜绿假单胞菌对各种抗菌药物的耐药率均在12.0%以下；鲍曼不动杆菌对头孢克肟和头孢噻肟耐药率均为7.1%，未发现对替加环素耐药的鲍曼不动杆菌。CNS中84.7%（83/98）为耐甲氧西林凝固酶阴性葡萄球菌（MRCNS）。金黄色葡萄球菌中43.5%（10/23）为耐甲氧西林金黄色葡萄球菌（MRSA）。未发现对万古霉素、利奈唑胺、替加环素耐药的G+菌。结论福建医科大学附属协和医院血液恶性肿瘤患者化疗后合并血流感染病原菌种类分布较广，以G−菌为主，耐药情况较严峻。临床上对怀疑有G+菌血液感染的患者可经验性选择万古霉素、利奈唑胺或替加环素抗感染治疗。
Published: 2017

50. Observation of the helicity-selection-rule suppressed decay of the χc2 charmonium state

Author: Y. Ding, H. R. Qi, X. N. Ma, B. J. Liu, I. Tapan, P. L. Wang, Y. P. Guo, Y. H. Yan, Q. Liu, Tristan Weber, Serkant Ali Cetin, J. Min, M. Savri, L. L. Ma, J. W. Zhao, L. Gong, L. G. Xia, A. Amoroso, B. Wang, M. Fritsch, Z. Y. You, Z. A. Zhu, F. A. Harris, Z. P. Zhang, H. Leithoff, Manuel Lara, H. B. Liu, Jie Zhao, D. X. Lin, X. L. Ji, Y. C. Zhu, C. Leng, M. Kavatsyuk, Y. J. Mao, H. X. Yang, Alexey Zhemchugov, H. M. Hu, I. Garzia, Ke Wang, H. Liang, Q. P. Ji, F. H. Liu, Nicolas Berger, C. P. Shen, H. Xiao, Z. Y. Zhang, A. Dbeyssi, R. Farinelli, H. L. Ma, B. Kopf, K. L. He, B. X. Zhang, Y. H. Guan, S. B. Liu, Y. Nefedov, J. W. Zhang, I. B. Nikolaev, J. H. Yin, M. Kornicer, D. M. Li, Zhiqing Liu, T. Held, H. Muramatsu, S. W. Han, L. H. Wu, A. Julin, Q. Ouyang, F. De Mori, R. Poling, P. F. Duan, F. H. Heinsius, W. Khn, Y. G. Xie, M. Shao, Y. T. Gu, P. Kiese, J. F. Sun, Fenfen An, Jimin Zhao, J. P. Liu, X. Y. Zhou, S. S. Fang, J. F. Chang, B. L. Wang, Z. L. Dou, L. J. Wu, S. Marcello, Y. Zeng, R. A. Briere, Zhe Sun, X. Q. Hao, F. Li, Y. F. Wang, E. H. Thorndike, F. C. Ma, S. Qian, Q. An, Jialun Ping, Jiaxi Liu, L. D. Liu, D. J. Ambrose, X. S. Jiang, E. Fioravanti, J. G. Messchendorp, Y. B. Liu, C. F. Redmer, T. C. Zhao, O. B. Kolcu, K. Zhang, Y. J. Mo, X. H. Liu, L. Q. Qin, M. Bertani, X. Cai, Xiao-Rui Lyu, P. Larin, Yao Wang, X. Y. Zhang, Q. A. Malik, G. Mezzadri, W. C. Yan, Qiunan Xu, Y. B. Zhao, H. B. Li, B. Kloss, C. L. Luo, Z. Haddadi, X. F. Wang, J. P. Dai, M. Pelizaeus, W. Shan, Q. M. Ma, X. L. Kang, A. Sarantsev, D. H. Wei, P. R. Li, J. S. Lange, Q. W. Zhao, L. Yang, O. Cakir, Y. B. Chen, Xiaofeng Zhu, J. Z. Zhang, G. S. Varner, S. Z. Chen, J. Q. Zhang, J. B. Liu, X. C. Chen, J. J. Xu, Z. H. Wang, M. N. Achasov, X. L. Gao, L. P. Zhou, R. Baldini Ferroli, X. Y. Niu, Y. Yuan, Y. S. Zhu, M. Albrecht, Y. J. Sun, E. Boger, C. C. Zhang, B. Zhong, L. B. Guo, Y. M. Ma, S. Ahmed, Y. X. Yang, Magnus Wolke, J. F. Qiu, W. G. Li, A. G. Denig, P. Musiol, Z. Ning, Xiaocong Ai, Z. P. Mao, J. Dong, Y. F. Liang, X. Fang, J. S. Huang, C. Schnier, Y. Q. Wang, W. D. Li, Krisztian Peters, Yu Zhang, Y. P. Lu, X. L. Luo, M. Z. Wang, M. H. Ye, Lei Li, T. Hussain, F. Feldbauer, X. Y. Ma, J. Fang, Tao Li, L. Fava, D. P. Jin, Z. L. Huang, Feng Liu, C. X. Liu, S. Spataro, X. T. Huang, S. Q. Zhang, Bibo Ke, W. Gradl, W. X. Gong, G. Rong, M. Ablikim, H. J. Lu, J. G. Lu, Y. Y. Liu, Cui Li, X. N. Li, I. R. Boyko, X. Y. Jiang, D. Y. Wang, C. Dong, Ch. Rosner, X. K. Zhou, A. Hafner, Q. Zhao, Haiping Peng, F. Nerling, J. B. Jiao, W. B. Yan, Y. Z. Sun, S. Sosio, S. Nisar, L. Y. Dong, C. J. Tang, Y. Hu, T. Ma, Liqing Xu, X. Y. Shen, A. A. Zafar, Yaquan Fang, M. Greco, X. H. Sun, M. Qi, H. H. Liu, Walter Ikegami Andersson, H. M. Liu, Y. X. Xia, H. J. Yang, N. Qin, K. Goetzen, Shou-hua Zhu, W. P. Wang, W. J. Zheng, F. Bianchi, F. E. Maas, J. C. Li, Y. H. Zheng, Tao Luo, Z. Gao, S. L. Niu, K. H. Rashid, Cong-Feng Qiao, O. Albayrak, G. F. Cao, Gang Zhao, I. Uman, X. Q. Li, Y. F. Long, T. Hu, J. Zhuang, N. Yu. Muchnoi, X. S. Kang, B. X. Yu, Zhi Zeng, M. X. Luo, Q. Y. Li, B. S. Zou, Y. T. Liang, Joachim Pettersson, Y. N. Guo, S. J. Chen, Y. H. Zhang, A. Q. Guo, L. Zotti, T. Holtmann, X. L. Li, D. V. Dedovich, O. Bakina, S. L. Olsen, K. J. Li, D. Xiao, W. M. Song, Z. Y. Wang, J. Y. Liu, Yunlong Zhang, F. Y. Li, H. S. Chen, Alperen Yuncu, Z. J. Xiao, X. H. Mo, Jin Li, D. Bettoni, H. L. Dai, K. Y. Liu, L. S. Wang, Z. B. Li, J. L. Zhang, S. Pacetti, Tord Johansson, Jianping Zheng, Z. H. Qin, S. Zhu, D. Y. Liu, Q. Gao, G. F. Xu, S. Jin, Y. N. Gao, L. L. Wang, H. Cai, Y. Zhang, G. S. Huang, P. X. Shen, Z. Wu, L. W. Jiang, S. X. Du, Xiaozhong Huang, J. Z. Fan, A. Calcaterra, Z. G. Zhao, Zhiqing Zhang, Jun-Yi Zhang, J. J. Zhang, M. Destefanis, X. Y. Song, H. H. Zhang, Z. J. Sun, H. Loehner, Andrzej Kupsc, C. Hu, X. Tang, Dan Wang, M. L. Chen, G. Felici, K. J. Zhu, D. W. Bennett, G. R. Liao, Zujian Wang, M. Y. Dong, H. J. Li, Q. L. Xiu, J. H. Zou, M. M. Ma, S. S. Sun, R. E. Mitchell, Fang Liu, U. Wiedner, I. Denysenko, J. Chai, G. X. Sun, J. V. Bennett, Li Yan, B. Y. Zhang, Z. Jiao, D. H. Zhang, J. Z. Bai, X. P. Xu, X. B. Ji, M. Tiemens, Y. H. Xie, M. Maggiora, Ling Zhao, Lei Zhao, Z. L. Hou, X. K. Chu, Z. G. Wang, H. Y. Zhang, P. Patteri, G. F. Chen, C. Z. Yuan, J. Y. Zhang, Peilian Liu, Lingxuan Zhang, Y. K. Heng, G. A. Chelkov, Karin Schönning, G. Li, Xichao Ruan, Yang Li, C. D. Fu, C. Q. Feng, X. R. Chen, M. G. Zhao, R. P. Guo, M. H. Gu, Z. Y. Deng, M. Ripka, H. Y. Sheng, Y. N. Zhang, J. M. Bian, S. J. Zhao, Q. J. Xu, C. X. Yu, J. C. Chen, Xuanhong Lou, Nasser Kalantar-Nayestanaki, C. Morales Morales, Yue Pan, R. Kliemt, Jie Yu, T. J. Min, B. Zheng, R. G. Ping, G. Cibinetto, Z. A. Liu, V. Prasad, Y. Ban, P. Weidenkaff, S. P. Wen, X. S. Qin, X. R. Zhou, and Cheng Li
Subjects: Physics, Particle physics, Meson, 010308 nuclear & particles physics, Electron–positron annihilation, 01 natural sciences, Helicity, Pseudoscalar meson, Nuclear magnetic resonance, Isospin, 0103 physical sciences, Pi, Intermediate state, Vector meson, 010306 general physics
Abstract: The decays of chi(c2) -> K+K- pi(0), KSK +/-pi(-/+), and pi(+)pi(-)pi(0) are studied with the psi(3686) data samples collected with the Beijing Spectrometer ( BESIII). For the first time, the br ...
Published: 2017

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