Institutional Repository of Radio Astronomy Research Laboratory
| A Single-pulse Study of PSR J1022+1001 Using the FAST Radio Telescope | |
Feng, Yi1,2,3; Hobbs, G.3; Li, D.1,2,4; Dai, S.3; Zhu, W. W.1; Yue, Y. L.1; Wang, P.1; Zhang, S. -B.2,3,5; Qian, L.1; Zhang, L.1,2,3; Wang, S. Q.6 ; Miao, C. C.1,2; Yuan, M.1,2; Zhang, Y. -K.1,2
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| 2021-02-01 | |
| Source Publication | ASTROPHYSICAL JOURNAL
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| ISSN | 0004-637X |
| Volume | 908Issue:1Pages:105 |
| Contribution Rank | 6 |
| Abstract | Using the Five-hundred-meter Aperture Spherical radio Telescope (FAST), we have recorded similar to 10(5) single pulses from PSR J1022+1001. We studied the polarization properties, their energy distribution, and their times of arrival. This is only possible with the high sensitivity available using FAST. There is no indication that PSR J1022+1001 exhibits giant pulse, nulling, or traditional mode changing phenomena. The energy in the leading and trailing components of the integrated profile is shown to be correlated. The degree of both linear and circular polarization increases with the pulse flux density for individual pulses. Our data indicates that pulse jitter leads to an excess noise in the timing residuals of 67 ns when scaled to one hour, which is consistent with Liu et al. We have unsuccessfully trialed various methods to improve timing precision through the selection of specific single pulses. Our work demonstrates that FAST can detect individual pulses from pulsars that are observed in order to detect and study gravitational waves. This capability enables detailed studies, and parameterization, of the noise processes that affect the sensitivity of a pulsar timing array. |
| Keyword | Pulsars Astronomy data analysis |
| DOI | 10.3847/1538-4357/abd326 |
| Indexed By | SCI |
| Language | 英语 |
| Funding Project | National Key R&D Program of China[2017YFA0402600] ; CAS International Partnership Program[114- A11KYSB20160008] ; CAS Strategic Priority Research Program[XDB23000000] ; NSFC[11725313] ; NSFC[11690024] ; China Scholarship Council |
| WOS Research Area | Astronomy & Astrophysics |
| WOS Subject | Astronomy & Astrophysics |
| WOS ID | WOS:000619557000001 |
| Publisher | IOP PUBLISHING LTD |
| Funding Organization | National Key R&D Program of China ; CAS International Partnership Program ; CAS Strategic Priority Research Program ; NSFC ; China Scholarship Council |
| Citation statistics | |
| Document Type | 期刊论文 |
| Identifier | http://ir.xao.ac.cn/handle/45760611-7/3854 |
| Collection | 射电天文研究室_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 |
| Corresponding Author | Feng, Yi |
| Affiliation | 1.Chinese Acad Sci, Natl Astron Observ, CAS Key Lab FAST, Beijing 100101, Peoples R China 2.Univ Chinese Acad Sci, Beijing 100049, Peoples R China 3.CSIRO Astron & Space Sci, POB 76, Epping, NSW 1710, Australia 4.Univ KwaZulu Natal, NAOC UKZN Computat Astrophys Ctr, Durban 4000, South Africa 5.Chinese Acad Sci, Purple Mt Observ, Nanjing 210008, Peoples R China 6.Xinjiang Astron Observ, 150,Sci 1 St, Xinjiang 830011, Peoples R China |
| Recommended Citation GB/T 7714 | Feng, Yi,Hobbs, G.,Li, D.,et al. A Single-pulse Study of PSR J1022+1001 Using the FAST Radio Telescope[J]. ASTROPHYSICAL JOURNAL,2021,908(1):105. |
| APA | Feng, Yi.,Hobbs, G..,Li, D..,Dai, S..,Zhu, W. W..,...&Zhang, Y. -K..(2021).A Single-pulse Study of PSR J1022+1001 Using the FAST Radio Telescope.ASTROPHYSICAL JOURNAL,908(1),105. |
| MLA | Feng, Yi,et al."A Single-pulse Study of PSR J1022+1001 Using the FAST Radio Telescope".ASTROPHYSICAL JOURNAL 908.1(2021):105. |
| Files in This Item: | ||||||
| File Name/Size | DocType | Version | Access | License | ||
| Feng-2021-A Single-p（1191KB） | 期刊论文 | 出版稿 | 开放获取 | CC BY-NC-SA | View Application Full Text | |
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