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Pulsar timing observations with Haoping Radio Telescope

文献类型：期刊论文

作者Luo, Jin-Tao2,3; Gao, Yu-Ping1,3; Yang, Ting-Gao3; Zhao, Cheng-Shi3; Tong, Ming-Lei3; Rao, Yong-Nan2,3; Li, Yi-Feng2,3; Li, Bian3; Zhu, Xing-Zhi3; Qiao, Hai-Hua3
刊名RESEARCH IN ASTRONOMY AND ASTROPHYSICS
出版日期2020-07-01
卷号20期号:7页码:6
关键词radio telescopes instrumentation miscellaneous methods data analysis pulsars general
ISSN号1674-4527
DOI10.1088/1674-4527/20/7/111
英文摘要We report pulsar timing observations carried out inL-band with NTSC's 40-meter Haoping Radio Telescope (HRT), which was constructed in 2014. These observations were carried out using the pulsar machine we developed. Timing observations toward millisecond pulsar J0437-4715 obtain a timing residual (r.m.s.) of 397 ns in the time span of 284 days. Our observations successfully detected Crab pulsar's glitch that happened on 2019 July 23.
资助项目Hundred Talents Program of the Chinese Academy of Sciences[Y650YC1201] ; National Natural Science Foundation of China[U1931128] ; National Natural Science Foundation of China[11973046] ; National Natural Science Foundation of China[91736207] ; National Natural Science Foundation of China[U1831130] ; National Natural Science Foundation of China[11903038] ; National Natural Science Foundation of China[11873050] ; National Natural Science Foundation of China[11873049] ; Natural Science Foundation of Shaanxi Province[2019JM-455] ; program of Youth Innovation Promotion Association CAS[2017450]
WOS研究方向Astronomy & Astrophysics
语种英语
WOS记录号WOS:000555744900001
出版者NATL ASTRONOMICAL OBSERVATORIES, CHIN ACAD SCIENCES
资助机构Hundred Talents Program of the Chinese Academy of Sciences ; Hundred Talents Program of the Chinese Academy of Sciences ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Natural Science Foundation of Shaanxi Province ; Natural Science Foundation of Shaanxi Province ; program of Youth Innovation Promotion Association CAS ; program of Youth Innovation Promotion Association CAS ; Hundred Talents Program of the Chinese Academy of Sciences ; Hundred Talents Program of the Chinese Academy of Sciences ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Natural Science Foundation of Shaanxi Province ; Natural Science Foundation of Shaanxi Province ; program of Youth Innovation Promotion Association CAS ; program of Youth Innovation Promotion Association CAS ; Hundred Talents Program of the Chinese Academy of Sciences ; Hundred Talents Program of the Chinese Academy of Sciences ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Natural Science Foundation of Shaanxi Province ; Natural Science Foundation of Shaanxi Province ; program of Youth Innovation Promotion Association CAS ; program of Youth Innovation Promotion Association CAS ; Hundred Talents Program of the Chinese Academy of Sciences ; Hundred Talents Program of the Chinese Academy of Sciences ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Natural Science Foundation of Shaanxi Province ; Natural Science Foundation of Shaanxi Province ; program of Youth Innovation Promotion Association CAS ; program of Youth Innovation Promotion Association CAS
源URL[http://210.72.145.45/handle/361003/9414]  
专题国家授时中心_守时理论与方法研究室
通讯作者Luo, Jin-Tao
作者单位1.Univ Chinese Acad Sci, Beijing 100049, Peoples R China
2.Chinese Acad Sci, Key Lab Precis Nav & Timing Technol, Xian 710600, Peoples R China
3.Chinese Acad Sci, Natl Time Serv Ctr, Xian 710600, Peoples R China
推荐引用方式
GB/T 7714		 Luo, Jin-Tao,Gao, Yu-Ping,Yang, Ting-Gao,et al. Pulsar timing observations with Haoping Radio Telescope[J]. RESEARCH IN ASTRONOMY AND ASTROPHYSICS,2020,20(7):6.
APA Luo, Jin-Tao.,Gao, Yu-Ping.,Yang, Ting-Gao.,Zhao, Cheng-Shi.,Tong, Ming-Lei.,...&Lu, Xiao-Chun.(2020).Pulsar timing observations with Haoping Radio Telescope.RESEARCH IN ASTRONOMY AND ASTROPHYSICS,20(7),6.
MLA Luo, Jin-Tao,et al."Pulsar timing observations with Haoping Radio Telescope".RESEARCH IN ASTRONOMY AND ASTROPHYSICS 20.7(2020):6.

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