The FAST Galactic Plane Pulsar Snapshot Survey - III. Timing results of 30 newly discovered pulsars
文献类型:期刊论文
作者 | Su, W. Q.1,2; Han, J. L.1,2,8; Wang, P. F.1,2,8; Yuan, J. P.7,8![]() |
刊名 | MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
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出版日期 | 2023-09-29 |
卷号 | 526期号:2页码:2645-2656 |
关键词 | pulsars: general |
ISSN号 | 0035-8711 |
DOI | 10.1093/mnras/stad2159 |
产权排序 | 4 |
英文摘要 | Timing observations are crucial for determining the basic parameters of newly discovered pulsars. Using the Five-hundred-meter Aperture Spherical radio Telescope (FAST) with the L-band 19-beam receiver covering the frequency range of 1.0-1.5 GHz, the FAST Galactic Plane Pulsar Snapshot (GPPS) Survey has discovered more than 600 faint pulsars with flux densities of only a few or a few tens of mu Jy at 1.25 GHz. To obtain accurate position, spin parameters and dispersion measure of a pulsar, and to calculate derived parameters such as the characteristic age and surface magnetic field, we collect available FAST pulsar data obtained either through targeted follow-up observations or through coincidental survey observations with one of the 19 beams of the receiver. From these data we obtain time of arrival (TOA) measurements for 30 newly discovered pulsars as well as for 13 known pulsars. We demonstrate that the TOA measurements acquired by the FAST from any beams of the receiver in any observation mode (e.g. the tracking mode or the snapshot mode) can be combined to get timing solutions. We update the ephemerides of 13 previously known pulsars and obtain the first phase-coherent timing results for 30 isolated pulsars discovered in the FAST GPPS Survey. Notably, PSR J1904+0853 is an isolated millisecond pulsar, PSR J1906+0757 is a disrupted recycled pulsar, and PSR J1856+0211 has a long period of 9.89 s that can constrain pulsar death lines. Based on these timing solutions, all available FAST data have been added together to obtain the best pulse profiles for these pulsars. |
WOS关键词 | CENTRAL COMPACT OBJECTS ; 2ND DATA RELEASE ; MILLISECOND PULSAR ; SPIN-DOWN ; RADIATION ; ACCELERATION ; SCATTERING ; GLITCHES ; ORIGIN ; RAY |
资助项目 | National Astronomical Observatories, Chinese Academy of Sciences ; Chinese Academy of Sciences[11988101] ; Chinese Academy of Sciences[11833009] ; National Natural Science Foundation of China (NSFC)[QYZDJ-SSW-SLH021] ; Key Research Program of the Chinese Academy of Sciences |
WOS研究方向 | Astronomy & Astrophysics |
语种 | 英语 |
WOS记录号 | WOS:001159221300054 |
出版者 | OXFORD UNIV PRESS |
资助机构 | National Astronomical Observatories, Chinese Academy of Sciences ; Chinese Academy of Sciences ; National Natural Science Foundation of China (NSFC) ; Key Research Program of the Chinese Academy of Sciences |
源URL | [http://ir.xao.ac.cn/handle/45760611-7/5876] ![]() |
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 | Han, J. L.; Wang, P. F. |
作者单位 | 1.Univ Chinese Acad Sci, Sch Astron & Space Sci, Beijing 100049, Peoples R China 2.Chinese Acad Sci, Natl Astron Observ, Jia 20 Datun Rd, Beijing 100012, Peoples R China 3.Southwest Univ, Sch Phys Sci & Technol, Chongqing 400715, Peoples R China 4.Peking Univ, Dept Astron, Beijing 100871, Peoples R China 5.Natl Astron Data Ctr, Guangzhou 510006, Guangdong, Peoples R China 6.Guangzhou Univ, Sch Phys & Mat Sci, Dept Astron, Guangzhou 510006, Guangdong, Peoples R China 7.Chinese Acad Sci, Xinjiang Astron Observ, 150 Sci 1 St, Urumqi 830011, Peoples R China 8.Chinese Acad Sci, Key Lab Radio Astron & Technol, Beijing 100101, Peoples R China |
推荐引用方式 GB/T 7714 | Su, W. Q.,Han, J. L.,Wang, P. F.,et al. The FAST Galactic Plane Pulsar Snapshot Survey - III. Timing results of 30 newly discovered pulsars[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2023,526(2):2645-2656. |
APA | Su, W. Q..,Han, J. L..,Wang, P. F..,Yuan, J. P..,Wang, Chen.,...&You, X. P..(2023).The FAST Galactic Plane Pulsar Snapshot Survey - III. Timing results of 30 newly discovered pulsars.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,526(2),2645-2656. |
MLA | Su, W. Q.,et al."The FAST Galactic Plane Pulsar Snapshot Survey - III. Timing results of 30 newly discovered pulsars".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 526.2(2023):2645-2656. |
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