FAST discovery of an extremely radio-faint millisecond pulsar from the Fermi-LAT unassociated source 3FGL J0318.1+0252
文献类型：期刊论文
| 作者 | Wang, Pei19; Li, Di18,19; Clark, Colin J.1,17; Parkinson, Pablo M. Saz14,15,16; Hou, Xian12,13; Zhu, Weiwei19; Qian, Lei19; Yue, Youling19; Pan, Zhichen19; Liu, Zhijie11 |
| 刊名 | SCIENCE CHINA-PHYSICS MECHANICS & ASTRONOMY
 |
| 出版日期 | 2021-12-01 |
| 卷号 | 64期号:12页码:8 |
| 关键词 | FAST pulsar radio gamma rays |
| ISSN号 | 1674-7348 |
| DOI | 10.1007/s11433-021-1757-5 |
| 通讯作者 | Wang, Pei(wangpei@nao.cas.cn) ; Li, Di(dili@nao.cas.cn) |
| 英文摘要 | High sensitivity radio searches of unassociated gamma-ray sources have proven to be an effective way of finding new pulsars. Using the Five-hundred-meter Aperture Spherical radio Telescope (FAST) during its commissioning phase, we have carried out a number of targeted deep searches of Fermi Large Area Telescope (LAT) gamma-ray sources. On February 27, 2018 we discovered an isolated millisecond pulsar (MSP), PSR J0318+0253, coincident with the unassociated gamma-ray source 3FGL J0318.1+0252. PSR J0318+0253 has a spin period of 5.19 ms, a dispersion measure (DM) of 26 pc cm(-3) corresponding to a DM distance of about 1.3 kpc, and a period-averaged flux density of (similar to 11 +/- 2) mu Jy at L-band (1.05-1.45 GHz). Among all high energy MSPs, PSR J0318+0253 is the faintest ever detected in radio bands, by a factor of at least similar to 4 in terms of L-band fluxes. With the aid of the radio ephemeris, an analysis of 9.6 years of Fermi-LAT data revealed that PSR J0318+0253 also displays strong gamma-ray pulsations. Follow-up observations carried out by both Arecibo and FAST suggest a likely spectral turn-over around 350 MHz. This is the first result from the collaboration between FAST and the Fermi-LAT teams as well as the first confirmed new MSP discovery by FAST, raising hopes for the detection of many more MSPs. Such discoveries will make a significant contribution to our understanding of the neutron star zoo while potentially contributing to the future detection of gravitational waves, via pulsar timing array (PTA) experiments. |
| WOS关键词 | TELESCOPE |
| 资助项目 | National Natural Science Foundation of China[11988101] ; National Natural Science Foundation of China[11690024] ; National Natural Science Foundation of China[11743002] ; National Natural Science Foundation of China[11873067] ; National Natural Science Foundation of China[U1631132] ; National Natural Science Foundation of China[U1831131] ; National Natural Science Foundation of China[U1731238] ; National Natural Science Foundation of China[U1938103] ; National Natural Science Foundation of China[11703047] ; National Natural Science Foundation of China[11773041] ; National Natural Science Foundation of China[11673060] ; National Key R&D Program of China[2017YFA0402600] ; Chinese Academy of Sciences (CAS) Key Laboratory of FAST, NAOC, Chinese Academy of Sciences ; National Basic Research Program of China[2015CB857100] ; CAS Strategic Priority Research Program[XDB23000000] ; CAS International Partnership Program[114A11KYSB20160008] ; Open Project Program of the Key Laboratory of FAST, NAOC, Chinese Academy of Sciences ; Guizhou Provincial Key Laboratory of Radio Astronomy and Data Processing, Guizhou Normal University ; Youth Innovation Promotion Association CAS[2021055] ; CAS Project for Young Scientists in Basic Reasearch[YSBR-006] ; Cultivation Project for FAST Scientific Payoff and Research Achievement of CAMS-CAS ; CAS Light of West China Program ; National Aeronautics and Space Administration ; Department of Energy in the United States ; Commissariat 'a l'Energie Atomique ; Centre National de la Recherche Scientifique/Institut National de Physique Nucleaire et de Physique des Particules in France ; Agenzia Spaziale Italiana ; Istituto Nazionale di Fisica Nucleare in Italy ; Ministry of Education, Culture, Sports, Science and Technology (MEXT) ; High Energy Accelerator Research Organization (KEK) ; Japan Aerospace Exploration Agency (JAXA) in Japan ; K. A. Wallenberg Foundation ; Swedish Research Council ; Swedish National Space Board in Sweden ; Istituto Nazionale di Astrofisica in Italy ; Centre National d'Etudes Spatiales in France ; DOE[DE-AC02-76SF00515] ; Fermi Guest Observer Program[80NSSC18K1731] ; ERC under the European Union[715051] ; NASA |
| WOS研究方向 | Physics |
| 语种 | 英语 |
| WOS记录号 | WOS:000710406900001 |
| 出版者 | SCIENCE PRESS |
| 资助机构 | National Natural Science Foundation of China ; National Key R&D Program of China ; Chinese Academy of Sciences (CAS) Key Laboratory of FAST, NAOC, Chinese Academy of Sciences ; National Basic Research Program of China ; CAS Strategic Priority Research Program ; CAS International Partnership Program ; Open Project Program of the Key Laboratory of FAST, NAOC, Chinese Academy of Sciences ; Guizhou Provincial Key Laboratory of Radio Astronomy and Data Processing, Guizhou Normal University ; Youth Innovation Promotion Association CAS ; CAS Project for Young Scientists in Basic Reasearch ; Cultivation Project for FAST Scientific Payoff and Research Achievement of CAMS-CAS ; CAS Light of West China Program ; National Aeronautics and Space Administration ; Department of Energy in the United States ; Commissariat 'a l'Energie Atomique ; Centre National de la Recherche Scientifique/Institut National de Physique Nucleaire et de Physique des Particules in France ; Agenzia Spaziale Italiana ; Istituto Nazionale di Fisica Nucleare in Italy ; Ministry of Education, Culture, Sports, Science and Technology (MEXT) ; High Energy Accelerator Research Organization (KEK) ; Japan Aerospace Exploration Agency (JAXA) in Japan ; K. A. Wallenberg Foundation ; Swedish Research Council ; Swedish National Space Board in Sweden ; Istituto Nazionale di Astrofisica in Italy ; Centre National d'Etudes Spatiales in France ; DOE ; Fermi Guest Observer Program ; ERC under the European Union ; NASA |
| 源URL | [http://ir.xao.ac.cn/handle/45760611-7/4304]  |
| 专题 | 脉冲星研究团组 新疆天文台_110米口径全可动射电望远镜（SmART）_110米大口径全可动射电望远镜关键技术研究（973项目）_课题1：大样本射电天体的观测和前沿问题研究 科研仪器设备产出_我台利用FAST观测数据文章 |
| 通讯作者 | Wang, Pei; Li, Di |
| 作者单位 | 1.Univ KwaZulu Natal, NAOC UKZN Computat Astrophys Ctr, ZA-4000 Durban, South Africa 2.Univ Maryland, Dept Phys, College Pk, MD 20742 USA 3.Xinjiang Astron Observ, Urumqi 830011, Peoples R China 4.Chinese Acad Sci, Shanghai Astron Observ, Shanghai 200030, Peoples R China 5.US Naval Res Lab, Space Sci Div, Washington, DC 20375 USA 6.Univ Bordeaux, Ctr Etud Nucl Bordeaux Gradignan, IN2P3 CNRS, F-33175 Gradignan, France 7.NASA, GSFC, Greenbelt, MD 20771 USA 8.NASA, UMCP CRESST GSFC, Greenbelt, MD 20771 USA 9.Stanford Univ, Phys Dept, Stanford, CA 94305 USA 10.Guizhou Normal Univ, Sch Phys & Elect Sci, Guiyang 550001, Peoples R China |
| 推荐引用方式 GB/T 7714 | Wang, Pei,Li, Di,Clark, Colin J.,et al. FAST discovery of an extremely radio-faint millisecond pulsar from the Fermi-LAT unassociated source 3FGL J0318.1+0252[J]. SCIENCE CHINA-PHYSICS MECHANICS & ASTRONOMY,2021,64(12):8. |
| APA | Wang, Pei.,Li, Di.,Clark, Colin J..,Parkinson, Pablo M. Saz.,Hou, Xian.,...&Wang, Na.(2021).FAST discovery of an extremely radio-faint millisecond pulsar from the Fermi-LAT unassociated source 3FGL J0318.1+0252.SCIENCE CHINA-PHYSICS MECHANICS & ASTRONOMY,64(12),8. |
| MLA | Wang, Pei,et al."FAST discovery of an extremely radio-faint millisecond pulsar from the Fermi-LAT unassociated source 3FGL J0318.1+0252".SCIENCE CHINA-PHYSICS MECHANICS & ASTRONOMY 64.12(2021):8. |
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