The FAST Galactic Plane Pulsar Snapshot survey - IV. Discovery of five fast radio bursts

被引:4
|
作者
Zhou, D. J. [1 ,2 ]
Han, J. L. [1 ,2 ,3 ]
Jing, W. C. [1 ,2 ]
Wang, P. F. [1 ,2 ]
Wang, C. [1 ,2 ]
Wang, T. [1 ,2 ]
Wang, W-Y [2 ,4 ,5 ,6 ]
Luo, R. [7 ,8 ]
Xu, J. [1 ]
Xu, R. X. [10 ]
Wang, H. G. [9 ,11 ]
机构
[1] Chinese Acad Sci, Natl Astron Observ, Jia-20 Datun Rd, Beijing 100101, Peoples R China
[2] Univ Chinese Acad Sci, Sch Astron, Beijing 100049, Peoples R China
[3] Chinese Acad Sci, CAS Key Lab FAST, NAOC, Beijing 100101, Peoples R China
[4] Peking Univ, Sch Phys, Beijing 100871, Peoples R China
[5] Peking Univ, State Key Lab Nucl Phys & Technol, Beijing 100871, Peoples R China
[6] Peking Univ, Kavli Inst Astron & Astrophys, Beijing 100871, Peoples R China
[7] CSIRO Space & Astron, POB 76, Epping, NSW 1710, Australia
[8] Guangzhou Univ, Sch Phys & Mat Sci, Dept Astron, Guangzhou 510006, Peoples R China
[9] Peking Univ, Dept Astron, Beijing 100871, Peoples R China
[10] Peking Univ, Dept Astron, Beijing 100871, Peoples R China
[11] Natl Astron Data Ctr, Great Bay Area, Guangzhou 510006, Peoples R China
基金
中国国家自然科学基金;
关键词
fast radio bursts; surveys; INTERSTELLAR SCATTERING; DEPENDENCE;
D O I
10.1093/mnras/stad2769
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We report five new fast radio bursts (FRBs) discovered from the Galactic Plane Pulsar Snapshot (GPPS) survey by the Five-hundred-meter Aperture Spherical radio Telescope (FAST): FRB 20210126, FRB 20210208, FRB 20210705, FRB 20211005, and FRB 20220306. To date, no repeating bursts from these FRB sources have been detected in the follow-up monitoring observations, leading to their classification as potential one-off events. We obtain the basic parameters for these bursts, including position, dispersion measure, pulse width, spectral index, scattering time-scale, etc. The fluences and flux densities are generally lower in comparison to the values observed in one-off bursts discovered by other telescopes. Among the observed bursts, polarization data for four bursts were recorded during observations. Consequently, we obtain polarization profiles and Faraday rotation measures for these bursts.
引用
收藏
页码:2657 / 2664
页数:8
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