Prospects for a multi-TeV gamma-ray sky survey with the LHAASO water Cherenkov detector array

doi:10.1088/1674-1137/44/6/065001

YNAO OpenIR > 南方基地

	Prospects for a multi-TeV gamma-ray sky survey with the LHAASO water Cherenkov detector array
	Aharonian, F.27,28; Alekseenko, V 24; An, Q.4; Axikegu 18; Bai, L. X.19; Bao, Y. W.14; Bastieri, D.9; Bi, X. J.1,2,3; Cai, H.21; Cao, Zhe 4; Cao, Zhen 1,2,3; Chang, J.15; Chang, J. F.1,3; Chang, X. C.1,3; Chao, S. P.1,16; Chen, B. M.1,12; Chen, J.19; Chen, L.1,3,17; Chen, M. L.1,3; Chen, M. J.1,3; Chen, Q. H.18; Chen, S. H.1,3; Chen, S. Z.1,3; Chen, T. L.20; Chen, X. L.1,3; Chen, Y.14; Cheng, N.1,3; Cheng, Y. D.1,3; Cui, S. W.12; Cui, X. H.6; Cui, Y. D.10; Dai, B. Z.22; Dai, H. L.1,3; Dai, Z. G.14; Danzengluobu 20; Piazzoli, B. D'Ettorre 29; Fang, J.22; Fan, J. H.9; Fan, Y. Z.15; Feng, C. F.16; Feng, L.15; Feng, S. H.1,3; Feng, Y. L.1,15; Gao, B.1,3; Gao, Q.20; Gao, W.16; Ge, M. M.22; Geng, L. S.1,3; Gong, G. H.5; Gou, Q. B.1,3; Gu, M. H.1,3; Guo, Y. Q.1,3; Guo, Y. Y.1,2,3; Han, Y. A.13; He, H. H.1,2,3; He, J. C.1,3; Heller, M.25; He, S. L.9; He, Y.18; Hou, C.1,3; Huang, D. H.18; Huang, Q. L.1,3; Huang, W. H.16; Huang, X. T.16; Hu, H. B.1,2,3; Hu, S.19; Jia, H. Y.18; Jiang, K.4; Ji, F.1,3; Jin, C.1,3; Ji, X. L.1,3; Levochkin, K.24; Liang, E. W.11; Liang, Y. F.11; Li, Cheng 4; Li, Cong 1,3; Li, F.1,3; Li, H.12; Li, H. B.1,3; Li, H. C.1,3; Li, H. M.5; Li, J.1,3; Li, K.1,3; Li, W. L.16; Li, X.1,18; Li, X. R.1,3; Li, Y.19; Li, Z.1,3,8; Liu, B.14; Liu, C.1,3; Liu, D.16; Liu, H. D.13; Liu, H.18; Liu, J.1,3; Liu, J. Y.1,3; Liu, M. Y.20; Liu, R. Y.14; Liu, S. M.15; Liu, W.1,3; Liu, Y. N.5; Liu, Z. X.19; Long, W. J.18; Lu, R.22; Lv, H. K.1,3; Mao JR(毛基荣)23 ; Masood, A.18; Mitthumsiri, W.26; Montaruli, T.25; Nan, Y. C.1,16; Pattarakijwanich, P.26; Pei, Z. Y.9; Qiao, B. Q.1,15; Qi, M. Y.1,3; Ruffolo, D.26; Rulev, V 24; Siz, A.26; Shao, L.12; Shchegolev, O.24; Sheng, X. D.1,3; Shi, J. R.1,3; Stenkin, Y.24; Stepanov, V 24; Sun, Z. B.7; Tam, P. H. T.10; Tang, Z. B.4; Tian, W. W.6; Volpe, D. D.25; Wang, C.7; Wang, H.18; Wang, H. G.9; Wang JC(王建成)23 ; Wang, L. Y.1,3; Wang, W.10,21; Wang, X. G.11; Wang, X. Y.14; Wang, X. J.1,3; Wang, Y. D.1,3; Wang, Y. J.1,3; Wang, Y. N.18; Wang, Y. P.1,3; Wang, Z.1,3; Wang, Z. H.19; Wang, Z. X.17; Wei, D. M.15; Wei, J. J.15; Wen, T.22; Wu, C. Y.1,3; Wu, H. R.1,3; Wu, S.1,3; Wu, W. X.18; Wu, X. F.15; Xiang, G. M.1,17; Xiao, G.1,3; Xin, G. G.1,21; Xing, Y.17; Xu, R. X.8; Xue, L.16; Yan DH(闫大海)23 ; Yang, C. W.19; Yang, F. F.1,3; Yang, L. L.10; Yang, M. J.1,3; Yang, R. Z.4; Yang, S. B.22; Yao, Y. H.1,19; Yao, Z. G.1,3; Ye, Y. M.5; Yin, L. Q.1,3; Yin, N.16; You, X. H.1,3; You, Z. Y.1,3; Yuan, Q.15; Yu, Y. H.16; Jiang, Z. J.22; Zeng, H. D.15; Zeng, T. X.1,3; Zeng, W.22; Zeng, Z. K.1,3; Zha, M.1,3; Zhang, B. B.14; Zhang, H. M.14; Zhang, H. Y.16; Zhang, J. L.6; Zhang, J. W.19; Zhang, L.22; Zhang, P. F.22; Zhang, P. P.12; Zhang, S. R.12; Zhang, S. S.1,3; Zhang, X.14; Zhang, X. P.1,3; Zhang, Yi 1,3; Zhang, Yong 1,3; Zhang, Y. F. G.18; Zhao, B.1,18; Zhao, J.1,3; Zhao, L.4; Zhao, L. Z.12; Zheng, F.7; Zheng, Y.18; Zhou, J. N.17; Zhou, P.14; Zhou, R.19; Zhou, X. X.18; Zhu, C. G.16; Zhu, F. R.18; Zhu, H.6; Zhu, K. J.1,3; Zuo, X.1,3
发表期刊	CHINESE PHYSICS C
	2020-06-01
卷号	44 期号:6 页码:10
DOI	10.1088/1674-1137/44/6/065001
产权排序	第23完成单位
收录类别	SCI
关键词	TeV gamma-ray astronomy observational prospect LHAASO-WCDA
摘要	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. WCDA is aimed at the study of TeV gamma-rays. In order to evaluate the prospects of searching for TeV gamma-ray sources with WCDA, we present a projection of the one-year sensitivity of WCDA to TeV gamma-ray sources from TeVCat using an all-sky approach. Out of 128 TeVCat sources observable by WCDA up to a zenith angle o 45 degrees f, we estimate that 42 would be detectable in 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).
资助项目	National Natural Science Foundation of China[11761141001] ; National Natural Science Foundation of China[11635011] ; National Natural Science Foundation of China[11873005] ; National Key R&D Program of China[2018YFA0404200] ; Chinese Academy of Sciences ; Key Laboratory of Particle Astrophysics, IHEP, CAS
项目资助者	National Natural Science Foundation of China[11761141001, 11635011, 11873005] ; National Key R&D Program of China[2018YFA0404200] ; Chinese Academy of Sciences ; Key Laboratory of Particle Astrophysics, IHEP, CAS
语种	英语
学科领域	物理学 ; 天文学
文章类型	Article
出版者	IOP PUBLISHING LTD
出版地	TEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND
ISSN	1674-1137
URL	查看原文
WOS记录号	WOS:000541791500001
WOS研究方向	Physics
WOS类目	Physics, Nuclear ; Physics, Particles & Fields
关键词[WOS]	HIGH-ENERGY ; DISCOVERY ; EMISSION ; SPECTRUM
引用统计	被引频次：6[WOS] [WOS记录] [WOS相关记录]
文献类型	期刊论文
条目标识符	http://ir.ynao.ac.cn/handle/114a53/23497
专题	南方基地
通讯作者	Chang, X. C.
作者单位	1.Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China 2.University of Chinese Academy of Sciences, Beijing 100049, China 3.TIANFU Cosmic Ray Research Center, Chengdu, Shichuan, China 4.University of Science and Technology of China, 230026 Hefei, Anhui, China 5.Tsinghua University, 100084 Beijing, China 6.National Astronomical Observatories, Chinese Academy of Sciences, 100101 Beijing, China 7.National Space Science Center, Chinese Academy of Sciences, 100190 Beijing, China 8.School of Physics, Peking University, 100871 Beijing, China 9.Center for Astrophysics, Guangzhou University, 510006 Guangzhou, Guangdong, China 10.Sun Yat-sen University, 519000 Zhuhai, Guangdong, China 11.Shool of Physics and Technology,Guangxi University, 530004 Nanning, Guangxi, China 12.Hebei Normal University, 050024 Shijiazhuang, Hebei, China 13.School of Physics and Engineering, Zhengzhou University, 450001 Zhengzhou, Henan, China 14.Nanjing University, 210023 Nanjing, Jiangsu, China 15.Key Laboratory of Dark Matter and Space Astronomy, Purple Mountain Observatory, Chinese Academy of Sciences, 210034 Nanjing, Jiangsu, China 16.Institute of Frontier and Interdisciplinary Science, Shandong University, 266237 Qingdao, Shandong, China 17.Shanghai Astronomical Observatory, Chinese Academy of Sciences, 200030 Shanghai, China 18.School of Physical Science and Technology, Southwest Jiaotong University, 610031 Chengdu, Sichuan, China 19.Sichuan University, 610065 Chengdu, Sichuan, China 20.Key Laboratory of Cosmic Rays (Tibet University), Ministry of Education, 850000 Lhasa, Tibet, China 21.School of physics and technology, Wuhan university, 430072 Wuhan, China 22.Yunnan University, 650091 Kunming,Yunnan,China 23.Yunnan Astronomical Observatories, Chinese Academy of Sciences, 650216 Kunming, Yunnan, China 24.Institute for Nuclear Research, Russian Academy of Sciences, Moscow, Russia 25.Département de Physique Nucléaire et Corpusculaire, Faculté de Sciences, Université de Genéve, Geneva, Switzerland 26.Department of Physics, Faculty of Science, Mahidol University, Bangkok, Thailand 27.Dublin Institute for Advanced Studies, 31 Fitzwilliam Place, Dublin 2, Ireland 28.Max-Planck-Institut fijr Kernphysik P.O. Box 103980, 69029 Heidelberg, Germany 29.Dipartimento di Fisica dell'Universit\`a di Napoli
推荐引用方式 GB/T 7714	Aharonian, F.,Alekseenko, V,An, Q.,et al. Prospects for a multi-TeV gamma-ray sky survey with the LHAASO water Cherenkov detector array[J]. CHINESE PHYSICS C,2020,44(6):10.
APA	Aharonian, F..,Alekseenko, V.,An, Q..,Axikegu.,Bai, L. X..,...&Zuo, X..(2020).Prospects for a multi-TeV gamma-ray sky survey with the LHAASO water Cherenkov detector array.CHINESE PHYSICS C,44(6),10.
MLA	Aharonian, F.,et al."Prospects for a multi-TeV gamma-ray sky survey with the LHAASO water Cherenkov detector array".CHINESE PHYSICS C 44.6(2020):10.

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