Institutional Repository System Of Yunnan Observatories, CAS
| The end-to-end Calibration of LHAASO-WFCTA based on Nitrogen Laser System | |
Sun, Qinning1; Min, Zhen2,3; Liu, Hu1; Chen, Long1; Wang, Yang1; Zhu, Fengrong1; Zhang, Shoushan2,3; Cao, Zhen2,4,5; Aharonian, F.6,7; An, Q.8,9; Axikegu10; Bai, L. X.11; Bai, Y. X.2,5; Bai, L. X.11; Bai, Y. X.2,5; Bao, Y. W.12; Bastieri, D.13; Bi, X. J.2,4,5; Bi, Y. J.2,5; Cai, H.14; Cai, J. T.13; Cao, Zhe8,9; Chang, J.15; Chang, J. F.2,5,8; Chen, B. M.16; Chen, E. S.2,4,5; Chen, J.11; Chen, Liang2,4,5; Chen, Liang17; Chen, Long10; Chen, M. J.2,5; Chen, M. L.2,5,8; Chen, Q. H.10; Chen, S. H.2,4,5; Chen, S. Z.2,5; Chen, T. L.18; Chen, X. L.2,4,5; Chen, Y.12; Cheng, N.2,5; Cheng, Y. D.2,5; Cui, S. W.16; Cui, X. H.19; Cui, Y. D.20; D’Ettorre Piazzoli, B.21; Dai, B. Z.22; Dai, H. L.2,5,8; Dai, Z. G.9; Danzengluobu18; della Volpe, D.23; Dong, X. J.2,5; Duan, K. K.15; Fan, J. H.13; Fan, Y. Z.15; Fan, Z. X.2,5; Fang, J.22; Fang, K.2,5; Feng, C. F.24; Feng, L.15; Feng, S. H.2,5; Feng, Y. L.15; Gao, B.2,5; Gao, C. D.24; Gao, L. Q.2,4,5; Gao, Q.18; Gao, W.24; Ge, M. M.22; Geng, L. S.2,5; Gong, G. H.25; Gou, Q. B.2,5; Gu, M. H.2,5,8; Guo, F. L.17; Guo, J. G.2,4,5; Guo, X. L.10; Guo, Y. Q.2,5; Guo, Y. Y.2,4,5,15; Han, Y. A.26; He, H. H.2,4,5; He, H. N.15; He, J. C.2,4,5; He, S. L.13; He, X. B.20; He, Y.10; Heller, M.23; Hor, Y. K.20; Hou, C.2,5; Hu, H. B.2,4,5; Hu, S.11; Hu, S. C.2,4,5; Hu, X. J.25; Huang, D. H.10; Huang, Q. L.2,5; Huang, W. H.24; Huang, X. T.24; Huang, X. Y.15; Huang, Z. C.10; Ji, F.5; Ji, X. L.2,5,8; Jia, H. Y.10; Jiang, K.8,9; Jiang, Z. J.22; Jin, C.2,4,5; Ke, T.2,5; Kuleshov, D.27; Levochkin, K.27; Li, B. B.16; Li, Cheng8,9; Li, Cong2,5; Li, F.2,5,8; Li, H. B.2,5; Li, H. C.2,5; Li, H. Y.9,15; Li, J.2,5,8; Li, K.2,5; Li, W. L.24; Li, X. R.2,5; Li, Xin8,9; Li, Xin10; Li, Y.11; Li, Y. Z.2,4,5; Li, Zhe2,5; Li, Zhuo28; Liang, E. W.29; Liang, Y. F.29; Lin, S. J.20; Liu, B.9; Liu, C.2,5; Liu, D.24; Liu, H.10; Liu, H. D.26; Liu, J.2,5; Liu, J. L.30; Liu, J. S.20; Liu, J. Y.2,5; Liu, M. Y.18; Liu, R. Y.12; Liu, S. M.10; Liu, W.2,5; Liu, Y.13; Liu, Y. N.25; Liu, Z. X.11; Long, W. J.10; Lu, R.22; Lv, H. K.2,5; Ma, B. Q.28; Ma, L. L.2,5; Ma, X. H.2,5; Mao JR(毛基荣)31 ; Masood, A.10; Min, Z.2,5; Mitthumsiri, W.32; Montaruli, T.23; Nan, Y. C.24; Pang, B. Y.10; Pattarakijwanich, P.32; Pei, Z. Y.13; Qi, M. Y.2,5; Qi, Y. Q.16; Qiao, B. Q.2,5; Qin, J. J.9; Ruffolo, D.32; Rulev, V.27; Sáiz, A.32; Shao, L.16; Shchegolev, O.27,33; Sheng, X. D.2,5; Shi, J. Y.2,5; Song, H. C.28; Stenkin, Yu. V.27,33; Stepanov, V.27; Su, Y.34; Sun, Q. N.10
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| 会议录名称 | Proceedings of Science |
| 2024-09-27 | |
| 卷号 | 444 |
| DOI | 10.22323/1.444.0494 |
| 产权排序 | 第31完成单位 |
| 收录类别 | EI |
| 会议名称 | 38th International Cosmic Ray Conference, ICRC 2023 |
| 会议日期 | 2023-07-26 |
| 会议地点 | Nagoya, Japan |
| 会议赞助商 | et al.; Institute for Cosmic Ray Research (ICRR) Univeristy of Tokyo; International Union of Pure and Applied Physics (IUPAP); JPS; Nagoya Convention and Visitors Bureau; Nagoya University |
| 摘要 | The Wide Field-of-view Cherenkov Telescope Array (WFCTA) of Large High Altitude Air Shower Observatory (LHAASO) is designed to perform nearly calorimetric measurements of extensive air showers induced by cosmic rays with energies between 1013 eV - 1018 eV. In order to achieve an end-to-end calibration of WFCTA and investigate properties of the atmospheric aerosol, five laser systems have been operated at LHAASO, including 3 nitrogen and 2 Nd:YAG laser devices. This work presents an overview of the laser signals received by the telescope and the monitoring of geometric information related to nitrogen laser events. Additionally, it introduces the simulation method for the LHAASO-WFCTA laser calibration system. Through prolonged and stable operation, a substantial amount of data has been accumulated, requiring further data analysis for the calibration of the telescope’s absolute gain and measurement of aerosol extinction coefficients. © Copyright owned by the author(s) under the terms of the Creative Commons. |
| 资助项目 | Science and Technology Department of Sichuan Province[2021YFSY0030];National Key Research and Development Program of China[2021YFA0718403];National Natural Science Foundation of China[12205244] |
| 项目资助者 | Science and Technology Department of Sichuan Province[2021YFSY0030] ; National Key Research and Development Program of China[2021YFA0718403] ; National Natural Science Foundation of China[12205244] |
| 语种 | 英语 |
| 学科领域 | 天文学 ; 天体物理学 ; 高能天体物理学 ; 星系与宇宙学 |
| 文章类型 | Conference article (CA) |
| URL | 查看原文 |
| EI入藏号 | 20245117555772 |
| EI主题词 | Cosmology |
| EI分类号 | 1301.1.3 - 1301.2.1.1.1 - 1302.1 - 1303.1 - 741.3 Optical Devices and Systems - 744.1 Lasers, General - 744.2 Gas Lasers - 941.9 - 942.1.11 |
| 引用统计 | |
| 文献类型 | 会议论文 |
| 条目标识符 | http://ir.ynao.ac.cn/handle/114a53/27927 |
| 专题 | 星系类星体研究组 |
| 作者单位 | 1.Southwest Jiaotong University, School of Physical Science and Technology, No. 999, Xi’an Road, Chengdu, China; 2.Institute of High Energy Physics, Chinese Academy of Sciences, Key Laboratory of Particle Astrophysics & Experimental Physics Division & Computing Center, No. 19B Yuquan Road, Beijing, 100049, China; 3.Institute of High Energy Physics, Chinese Academy of Sciences, TIANFU Cosmic Ray Research Center, No. 1500 Kezhi Road, Chengdu, China; 4.University of Chinese Academy of Sciences, Beijing, 100049, China; 5.TIANFU Cosmic Ray Research Center, Sichuan, Chengdu, China; 6.Dublin Institute for Advanced Studies, 31 Fitzwilliam Place, Dublin 2, Ireland; 7.Max-Planck-Institut for Nuclear Physics, P.O. Box 103980, Heidelberg, 69029, Germany; 8.State Key Laboratory of Particle Detection and Electronics, China; 9.University of Science and Technology of China, Anhui, Hefei, 230026, China; 10.School of Physical Science and Technology, School of Information Science and Technology, Southwest Jiaotong University, Sichuan, Chengdu, 610031, China; 11.College of Physics, Sichuan University, Sichuan, Chengdu, 610065, China; 12.School of Astronomy and Space Science, Nanjing University, Jiangsu, Nanjing, 210023, China; 13.Center for Astrophysics, Guangzhou University, Guangdong, Guangzhou, 510006, China; 14.School of Physics and Technology, Wuhan University, Hubei, Wuhan, 430072, China; 15.Key Laboratory of Dark Matter and Space Astronomy, Purple Mountain Observatory, Chinese Academy of Sciences, Jiangsu, Nanjing, 210023, China; 16.Hebei Normal University, Hebei, Shijiazhuang, 050024, China; 17.Key Laboratory for Research in Galaxies and Cosmology, Shanghai Astronomical Observatory, Chinese Academy of Sciences, Shanghai, 200030, China; 18.Key Laboratory of Cosmic Rays (Tibet University), Ministry of Education, Tibet, Lhasa, 850000, China; 19.National Astronomical Observatories, Chinese Academy of Sciences, Beijing, 100101, China; 20.School of Physics and Astronomy, School of Physics (Guangzhou), Sun Yat-sen University, Guangdong, Zhuhai, 519000, China; 21.Dipartimento di Fisica dell’Università di Napoli ‘Federico II", Complesso Universitario di Monte Sant’Angelo, via Cinthia, Napoli, 80126, Italy; 22.School of Physics and Astronomy, Yunnan University, Yunnan, Kunming, 650091, China; 23.D’epartement de Physique Nucl’eaire et Corpusculaire, Facult’e de Sciences, Universit’e de Gen‘eve, 24 Quai Ernest Ansermet, Geneva, 1211, Switzerland; 24.Institute of Frontier and Interdisciplinary Science, Shandong University, Shandong, Qingdao, 266237, China; 25.Department of Engineering Physics, Tsinghua University, Beijing, 100084, China; 26.School of Physics and Microelectronics, Zhengzhou University, Henan, Zhengzhou, 450001, China; 27.Institute for Nuclear Research of Russian Academy of Sciences, Moscow, 117312, Russia; 28.School of Physics, Peking University, Beijing, 100871, China; 29.School of Physical Science and Technology, Guangxi University, Guangxi, Nanning, 530004, China; 30.Tsung-Dao Lee Institute, School of Physics and Astronomy, Shanghai Jiao Tong University, Shanghai, 200240, China; 31.Yunnan Observatories, Chinese Academy of Sciences, Yunnan, Kunming, 650216, China; 32.Department of Physics, Faculty of Science, Mahidol University, Bangkok, 10400, Thailand; 33.Moscow Institute of Physics and Technology, Moscow, 141700, Russia; 34.Key Laboratory of Radio Astronomy, Purple Mountain Observatory, Chinese Academy of Sciences, Jiangsu, Nanjing, 210023, China; 35.National Space Science Center, Chinese Academy of Sciences, Beijing, 100190, China |
| 推荐引用方式 GB/T 7714 | Sun, Qinning,Min, Zhen,Liu, Hu,et al. The end-to-end Calibration of LHAASO-WFCTA based on Nitrogen Laser System[C],2024. |
| 条目包含的文件 | ||||||
| 文件名称/大小 | 文献类型 | 版本类型 | 开放类型 | 使用许可 | ||
| The end-to-end Calib（1178KB） | 会议论文 | 开放获取 | CC BY-NC-SA | 浏览 请求全文 | ||
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