The detection of an extremely bright fast radio burst in a phased array feed survey

K. W. Bannister; R. M. Shannon; J.-P. Macquart; C. Flynn; P. G. Edwards; M. O'Neill; S. Osłowski; M. Bailes; B. Zackay; N. Clarke; L. R. D'Addario; R. Dodson; P.J. Hall; A. Jameson; D. Jones; R. Navarro; J. T. Trinh; J. Allison; C. S. Anderson; M. Bell; A. P. Chippendale; J. D. Collier; G. Heald; I. Heywood; A. W. Hotan; K. Lee-Waddell; J. P. Madrid; J. Marvil; D. McConnell; A. Popping; M. A. Voronkov; M. T. Whiting; G. R. Allen; D. C.-J. Bock; D. P. Brodrick; F. Cooray; D. R. Deboer; P. J. Diamond; R. Ekers; R. G. Gough; G. A. Hampson; L. Harvey-Smith; S. G. Hay; D. B. Hayman; C. A. Jackson; S. Johnston; B. S. Koribalski; N. M. McClure-Griffiths; P. Mirtschin; A. Ng; R. P. Norris; S. E. Pearce; C. J. Phillips; D. N. Roxby; E. R. Troup; T. Westmeier

doi:10.3847/2041-8213/aa71ff

The detection of an extremely bright fast radio burst in a phased array feed survey

K. W. Bannister
, R. M. Shannon
, J.-P. Macquart
, C. Flynn
, P. G. Edwards
, M. O'Neill
, S. Osłowski
, M. Bailes
, B. Zackay
, N. Clarke
, L. R. D'Addario
, R. Dodson
, P.J. Hall
, A. Jameson
, D. Jones
, R. Navarro
, J. T. Trinh
, J. Allison
, C. S. Anderson
, M. Bell

A. P. Chippendale, J. D. Collier, G. Heald, I. Heywood, A. W. Hotan, K. Lee-Waddell, J. P. Madrid, J. Marvil, D. McConnell, A. Popping, M. A. Voronkov, M. T. Whiting, G. R. Allen, D. C.-J. Bock, D. P. Brodrick, F. Cooray, D. R. Deboer, P. J. Diamond, R. Ekers, R. G. Gough, G. A. Hampson, L. Harvey-Smith, S. G. Hay, D. B. Hayman, C. A. Jackson, S. Johnston, B. S. Koribalski, N. M. McClure-Griffiths, P. Mirtschin, A. Ng, R. P. Norris, S. E. Pearce, C. J. Phillips, D. N. Roxby, E. R. Troup, T. Westmeier

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159 Citations (Scopus)

Abstract

We report the detection of an ultra-bright fast radio burst (FRB) from a modest, 3.4-day pilot survey with the Australian Square Kilometre Array Pathfinder. The survey was conducted in a wide-field fly's-eye configuration using the phased-array-feed technology deployed on the array to instantaneously observe an effective area of 160 deg2, and achieve an exposure totaling 13200 deg2 hr . We constrain the position of FRB 170107 to a region in size (90% containment) and its fluence to be 58 Â±6 Jy ms. The spectrum of the burst shows a sharp cutoff above 1400 MHz, which could be due to either scintillation or an intrinsic feature of the burst. This confirms the existence of an ultra-bright (> Jy ms) population of FRBs.

Original language	English
Article number	L12
Number of pages	6
Journal	The Astrophysical Journal Letters
Volume	841
Issue number	1
DOIs	https://doi.org/10.3847/2041-8213/aa71ff
Publication status	Published - 2017

Keywords

radio astronomy
radio telescopes

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10.3847/2041-8213/aa71ff

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Bannister, K. W., Shannon, R. M., Macquart, J.-P., Flynn, C., Edwards, P. G., O'Neill, M., Osłowski, S., Bailes, M., Zackay, B., Clarke, N., D'Addario, L. R., Dodson, R., Hall, P. J., Jameson, A., Jones, D., Navarro, R., Trinh, J. T., Allison, J., Anderson, C. S., ... Westmeier, T. (2017). The detection of an extremely bright fast radio burst in a phased array feed survey. The Astrophysical Journal Letters, 841(1), Article L12. https://doi.org/10.3847/2041-8213/aa71ff

@article{84a57fb7a4344069917f4e7531291d17,

title = "The detection of an extremely bright fast radio burst in a phased array feed survey",

abstract = "We report the detection of an ultra-bright fast radio burst (FRB) from a modest, 3.4-day pilot survey with the Australian Square Kilometre Array Pathfinder. The survey was conducted in a wide-field fly's-eye configuration using the phased-array-feed technology deployed on the array to instantaneously observe an effective area of 160 deg2, and achieve an exposure totaling 13200 deg2 hr . We constrain the position of FRB 170107 to a region in size (90\% containment) and its fluence to be 58 {\^A}±6 Jy ms. The spectrum of the burst shows a sharp cutoff above 1400 MHz, which could be due to either scintillation or an intrinsic feature of the burst. This confirms the existence of an ultra-bright (> Jy ms) population of FRBs.",

keywords = "radio astronomy, radio telescopes",

author = "Bannister, \{K. W.\} and Shannon, \{R. M.\} and J.-P. Macquart and C. Flynn and Edwards, \{P. G.\} and M. O'Neill and S. Os{\l}owski and M. Bailes and B. Zackay and N. Clarke and D'Addario, \{L. R.\} and R. Dodson and P.J. Hall and A. Jameson and D. Jones and R. Navarro and Trinh, \{J. T.\} and J. Allison and Anderson, \{C. S.\} and M. Bell and Chippendale, \{A. P.\} and Collier, \{J. D.\} and G. Heald and I. Heywood and Hotan, \{A. W.\} and K. Lee-Waddell and Madrid, \{J. P.\} and J. Marvil and D. McConnell and A. Popping and Voronkov, \{M. A.\} and Whiting, \{M. T.\} and Allen, \{G. R.\} and Bock, \{D. C.-J.\} and Brodrick, \{D. P.\} and F. Cooray and Deboer, \{D. R.\} and Diamond, \{P. J.\} and R. Ekers and Gough, \{R. G.\} and Hampson, \{G. A.\} and L. Harvey-Smith and Hay, \{S. G.\} and Hayman, \{D. B.\} and Jackson, \{C. A.\} and S. Johnston and Koribalski, \{B. S.\} and McClure-Griffiths, \{N. M.\} and P. Mirtschin and A. Ng and Norris, \{R. P.\} and Pearce, \{S. E.\} and Phillips, \{C. J.\} and Roxby, \{D. N.\} and Troup, \{E. R.\} and T. Westmeier",

year = "2017",

doi = "10.3847/2041-8213/aa71ff",

language = "English",

volume = "841",

journal = "The Astrophysical Journal Letters",

issn = "2041-8205",

publisher = "Institute of Physics Publishing",

number = "1",

}

Bannister, KW, Shannon, RM, Macquart, J-P, Flynn, C, Edwards, PG, O'Neill, M, Osłowski, S, Bailes, M, Zackay, B, Clarke, N, D'Addario, LR, Dodson, R, Hall, PJ, Jameson, A, Jones, D, Navarro, R, Trinh, JT, Allison, J, Anderson, CS, Bell, M, Chippendale, AP, Collier, JD, Heald, G, Heywood, I, Hotan, AW, Lee-Waddell, K, Madrid, JP, Marvil, J, McConnell, D, Popping, A, Voronkov, MA, Whiting, MT, Allen, GR, Bock, DC-J, Brodrick, DP, Cooray, F, Deboer, DR, Diamond, PJ, Ekers, R, Gough, RG, Hampson, GA, Harvey-Smith, L, Hay, SG, Hayman, DB, Jackson, CA, Johnston, S, Koribalski, BS, McClure-Griffiths, NM, Mirtschin, P, Ng, A, Norris, RP, Pearce, SE, Phillips, CJ, Roxby, DN, Troup, ER & Westmeier, T 2017, 'The detection of an extremely bright fast radio burst in a phased array feed survey', The Astrophysical Journal Letters, vol. 841, no. 1, L12. https://doi.org/10.3847/2041-8213/aa71ff

TY - JOUR

T1 - The detection of an extremely bright fast radio burst in a phased array feed survey

AU - Bannister, K. W.

AU - Shannon, R. M.

AU - Macquart, J.-P.

AU - Flynn, C.

AU - Edwards, P. G.

AU - O'Neill, M.

AU - Osłowski, S.

AU - Bailes, M.

AU - Zackay, B.

AU - Clarke, N.

AU - D'Addario, L. R.

AU - Dodson, R.

AU - Hall, P.J.

AU - Jameson, A.

AU - Jones, D.

AU - Navarro, R.

AU - Trinh, J. T.

AU - Allison, J.

AU - Anderson, C. S.

AU - Bell, M.

AU - Chippendale, A. P.

AU - Collier, J. D.

AU - Heald, G.

AU - Heywood, I.

AU - Hotan, A. W.

AU - Lee-Waddell, K.

AU - Madrid, J. P.

AU - Marvil, J.

AU - McConnell, D.

AU - Popping, A.

AU - Voronkov, M. A.

AU - Whiting, M. T.

AU - Allen, G. R.

AU - Bock, D. C.-J.

AU - Brodrick, D. P.

AU - Cooray, F.

AU - Deboer, D. R.

AU - Diamond, P. J.

AU - Ekers, R.

AU - Gough, R. G.

AU - Hampson, G. A.

AU - Harvey-Smith, L.

AU - Hay, S. G.

AU - Hayman, D. B.

AU - Jackson, C. A.

AU - Johnston, S.

AU - Koribalski, B. S.

AU - McClure-Griffiths, N. M.

AU - Mirtschin, P.

AU - Ng, A.

AU - Norris, R. P.

AU - Pearce, S. E.

AU - Phillips, C. J.

AU - Roxby, D. N.

AU - Troup, E. R.

AU - Westmeier, T.

PY - 2017

Y1 - 2017

N2 - We report the detection of an ultra-bright fast radio burst (FRB) from a modest, 3.4-day pilot survey with the Australian Square Kilometre Array Pathfinder. The survey was conducted in a wide-field fly's-eye configuration using the phased-array-feed technology deployed on the array to instantaneously observe an effective area of 160 deg2, and achieve an exposure totaling 13200 deg2 hr . We constrain the position of FRB 170107 to a region in size (90% containment) and its fluence to be 58 Â±6 Jy ms. The spectrum of the burst shows a sharp cutoff above 1400 MHz, which could be due to either scintillation or an intrinsic feature of the burst. This confirms the existence of an ultra-bright (> Jy ms) population of FRBs.

AB - We report the detection of an ultra-bright fast radio burst (FRB) from a modest, 3.4-day pilot survey with the Australian Square Kilometre Array Pathfinder. The survey was conducted in a wide-field fly's-eye configuration using the phased-array-feed technology deployed on the array to instantaneously observe an effective area of 160 deg2, and achieve an exposure totaling 13200 deg2 hr . We constrain the position of FRB 170107 to a region in size (90% containment) and its fluence to be 58 Â±6 Jy ms. The spectrum of the burst shows a sharp cutoff above 1400 MHz, which could be due to either scintillation or an intrinsic feature of the burst. This confirms the existence of an ultra-bright (> Jy ms) population of FRBs.

KW - radio astronomy

KW - radio telescopes

UR - http://handle.westernsydney.edu.au:8081/1959.7/uws:41115

U2 - 10.3847/2041-8213/aa71ff

DO - 10.3847/2041-8213/aa71ff

M3 - Article

SN - 2041-8205

VL - 841

JO - The Astrophysical Journal Letters

JF - The Astrophysical Journal Letters

IS - 1

M1 - L12

ER -

The detection of an extremely bright fast radio burst in a phased array feed survey

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Keywords

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