A survey of the Galactic plane for dispersed radio pulses with the Australian Square Kilometre Array Pathfinder

被引:19
作者
Qiu, Hao [1 ,2 ]
Bannister, K. W. [2 ]
Shannon, R. M. [3 ,4 ]
Murphy, Tara [1 ]
Bhandari, Shivani [2 ]
Agarwal, Devansh [5 ,6 ]
Lorimer, D. R. [5 ,6 ]
Bunton, J. D. [2 ]
机构
[1] Univ Sydney, Sydney Inst Astrophys, Sch Phys, Sydney, NSW 2006, Australia
[2] Australia Telescope Natl Facil, CSIRO Astron & Space Sci, POB 76, Epping, NSW 1710, Australia
[3] Swinburne Univ Technol, Ctr Astrophys & Supercomp, Mail H30,POB 218, Hawthorn, Vic 3122, Australia
[4] ARC Ctr Excellence Gravitat Wave Discovery OzGrav, Hawthorn, Vic, Australia
[5] West Virginia Univ, Dept Phys & Astron, POB 6315, Morgantown, WV USA
[6] West Virginia Univ, Ctr Gravitat Waves & Cosmol, Chestnut Ridge Res Bldg, Morgantown, WV USA
基金
澳大利亚研究理事会; 美国国家科学基金会;
关键词
surveys; pulsars: general; ISM: structure; intergalactic medium; BURSTS; DISCOVERY; TRANSIENTS; ENERGETICS; EMISSION; PULSARS; EVENTS; LIMITS;
D O I
10.1093/mnras/stz748
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We report the results from a survey of the Galactic plane for dispersed single pulses using the Australian SKA Pathfinder (ASKAP). We searched for rare bright dispersed radio pulses comprising 160 pointings covering 4800 deg(2) of the Galactic plane within vertical bar b vertical bar < 7 degrees, each pointing with an exposure time of 10 h. We detected one fast radio burst, FRB 180430, and single pulses from 11 pulsars. No rotating radio transients were detected. We detected FRB 180430 in the Galactic plane in the anticentre direction with a fluence of 216 +/- 5 Jy ms a dispersion measure (DM) of 264.1 pc cm(-3). We estimate the extragalactic DM of the object to be less than 86.7 pc cm(-3) depending on the electron density model. One model suggests that this FRB may be a giant pulse within our galaxy; we discuss how this may not correctly represent the line-of-sight DM. Based on the single detection of FRB 180430 in 3.47 x 10(4) deg(2) h we derive an FRB event rate in the Galactic plane at the 20 Jy ms threshold to be in the range 2-140 per sky per day at 95 per cent confidence. Despite the necessarily large uncertainties from this single detection, this is consistent with the current ASKAP all-sky detection rate.
引用
收藏
页码:166 / 174
页数:9
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