中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Pulse Jitter and Single-pulse Variability in Millisecond Pulsars

文献类型:期刊论文

作者Wang, S. Q.6,7,9; Wang, N.6,7,9; Wang, J. B.8; Hobbs, G.4; Xu, H.1; Wang, B. J.1; Dai, S.2; Dang, S. J.3; Li, D.1; Feng, Y.5
刊名ASTROPHYSICAL JOURNAL
出版日期2024-03-01
卷号964期号:1页码:6
ISSN号0004-637X
DOI10.3847/1538-4357/ad217b
产权排序1
英文摘要Understanding the jitter noise resulting from single-pulse phase and shape variations is important for the detection of gravitational waves using pulsar timing arrays. We present measurements of the jitter noise and single-pulse variability of 12 millisecond pulsars that are part of the International Pulsar Timing Array sample using the Five-hundred-meter Aperture Spherical radio Telescope. We find that the levels of jitter noise can vary dramatically among pulsars. A moderate correlation with a correlation coefficient of 0.57 between jitter noise and pulse width is detected. To mitigate jitter noise, we perform matrix template matching using all four Stokes parameters. Our results reveal a reduction in jitter noise ranging from 6.7% to 39.6%. By performing longitude-resolved fluctuation spectrum analysis, we identify periodic intensity modulations in 10 pulsars. In PSR J0030+0451, we detect single pulses with energies more than 10 times the average pulse energy, suggesting the presence of giant pulses. We also observe a periodic mode-changing phenomenon in PSR J0030+0451. We examine the achievable timing precision by selecting a subset of pulses with a specific range of peak intensity, but no significant improvement in timing precision is achievable.
WOS关键词YR DATA SET ; FREQUENCY-DEPENDENCE ; DRIFTING SUBPULSES ; PRECISION ; POLARIMETRY ; MODULATION ; SEARCH ; LIMITS
资助项目the national natural science foundation of China[12288102] ; the national natural science foundation of China[12203092] ; the national natural science foundation of China[12041304] ; National Natural Science Foundation of China[2022A03013-3] ; National Natural Science Foundation of China[2022A03013-2] ; Major Science and Technology Program of Xinjiang Uygur Autonomous Region[2020SKA0120100] ; National SKA Program of China[2022YFC2205202] ; National SKA Program of China[2021YFC2203502] ; National Key Research and Development Program of China[2022D01B71] ; National Key Research and Development Program of China[2022D01D85] ; Natural Science Foundation of Xinjiang Uygur Autonomous Region[2023TSYCQNTJ0024] ; Tianshan Talent Training Program for Young Elite Scientists ; Special Research Assistant Program of CAS[YSBR-063] ; CAS Project for Young Scientists in Basic Research[2021PE0AC03] ; Key Research Project of Zhejiang Laboratory[LY23A030001] ; Zhejiang Provincial Natural Science Foundation of China ; Chinese Academy of Sciences ; Operation, Maintenance and Upgrading Fund for Astronomical Telescopes and Facility Instruments ; Ministry of Finance of China (MOF)
WOS研究方向Astronomy & Astrophysics
语种英语
WOS记录号WOS:001182066600001
出版者IOP Publishing Ltd
资助机构the national natural science foundation of China ; National Natural Science Foundation of China ; Major Science and Technology Program of Xinjiang Uygur Autonomous Region ; National SKA Program of China ; National Key Research and Development Program of China ; Natural Science Foundation of Xinjiang Uygur Autonomous Region ; Tianshan Talent Training Program for Young Elite Scientists ; Special Research Assistant Program of CAS ; CAS Project for Young Scientists in Basic Research ; Key Research Project of Zhejiang Laboratory ; Zhejiang Provincial Natural Science Foundation of China ; Chinese Academy of Sciences ; Operation, Maintenance and Upgrading Fund for Astronomical Telescopes and Facility Instruments ; Ministry of Finance of China (MOF)
源URL[http://ir.xao.ac.cn/handle/45760611-7/5914]  
专题脉冲星研究团组
科研仪器设备产出_我台利用FAST观测数据文章
通讯作者Wang, S. Q.
作者单位1.Chinese Acad Sci, Natl Astron Observ, Beijing 100101, Peoples R China
2.Western Sydney Univ, Sch Sci, Locked Bag 1797, Penrith, NSW 2751, Australia
3.Guizhou Normal Univ, Sch Phys & Elect Sci, Guiyang 550001, Peoples R China
4.CSIRO Astron & Space Sci, POB 76, Epping, NSW 1710, Australia
5.Zhejiang Lab, Hangzhou, Zhejiang, Peoples R China
6.Chinese Acad Sci, Key Lab Radio Astron, Urumqi 830011, Xinjiang, Peoples R China
7.Chinese Acad Sci, Xinjiang Astron Observ, Urumqi 830011, Xinjiang, Peoples R China
8.Lishui Univ, Inst Optoelect Technol, Lishui 323000, Zhejiang, Peoples R China
9.Xinjiang Key Lab Radio Astrophys, Urumqi 830011, Xinjiang, Peoples R China
推荐引用方式
GB/T 7714
Wang, S. Q.,Wang, N.,Wang, J. B.,et al. Pulse Jitter and Single-pulse Variability in Millisecond Pulsars[J]. ASTROPHYSICAL JOURNAL,2024,964(1):6.
APA Wang, S. Q..,Wang, N..,Wang, J. B..,Hobbs, G..,Xu, H..,...&Zhang, C. M..(2024).Pulse Jitter and Single-pulse Variability in Millisecond Pulsars.ASTROPHYSICAL JOURNAL,964(1),6.
MLA Wang, S. Q.,et al."Pulse Jitter and Single-pulse Variability in Millisecond Pulsars".ASTROPHYSICAL JOURNAL 964.1(2024):6.

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