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

**Authors:** Keith Bannister, Ryan Shannon, Jean-Pierre Macquart, Chris Flynn,, Philip Edwards, Morgan O'Neill, Stefan Os{\l}owski, Matthew Bailes, Barak, Zackay, Nathan Clarke, Larry D'Addario, Richard Dodson, Peter Hall, Andrew, Jameson, Dayton Jones, Robert Navarro, Joseph Trinh, James Allison, Craig, Anderson, Martin Bell, Aaron Chippendale, Jordan Collier, George Heald, Ian, Heywood, Aidan Hotan, Karen Lee-Waddell, Juan Madrid, Joshua Marvil, David, McConnell, Attila Popping, Maxim Voronkov, Matthew Whiting, Graham Allen,, Douglas Bock, David Brodrick, Francis Cooray, David DeBoer, Philip Diamond,, Ron Ekers, Russell Gough, Grant Hampson, Lisa Harvey-Smith, Stuart Hay,, Douglas Hayman, Carole Jackson, Simon Johnston, Baerbel Koribalski, Naomi, McClure-Griffiths, Peter Mirtschin, Alan Ng, Ray Norris, Sarah Pearce, Chris, Phillips, Daniel Roxby, Euan Robert Troup, Tobias Westmeier

arXiv: 1705.07581 · 2017-05-31

## TL;DR

This paper reports the discovery of an ultra-bright fast radio burst using the Australian Square Kilometre Array Pathfinder, demonstrating the effectiveness of wide-field phased-array-feed surveys in detecting bright FRBs.

## Contribution

It presents the first detection of an ultra-bright FRB with a wide-field phased-array-feed survey, highlighting the survey's capability to find bright FRBs efficiently.

## Key findings

- Detected an ultra-bright FRB with 58 Jy ms fluence.
- Constrained the FRB's position to an 8'x8' region.
- Observed a spectral cutoff above 1400 MHz.

## 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 $160$ deg$^2$, and achieve an exposure totaling $13200$ deg$^2$ hr. We constrain the position of FRB 170107 to a region $8'\times8'$ in size (90% containment) and its fluence to be $58\pm6$ Jy ms. The spectrum of the burst shows a sharp cutoff above $1400$ MHz, which could be either due to scintillation or an intrinsic feature of the burst. This confirms the existence of an ultra-bright ($>20$ Jy ms) population of FRBs.

## Full text

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## Figures

8 figures with captions in the complete paper: https://tomesphere.com/paper/1705.07581/full.md

## References

34 references — full list in the complete paper: https://tomesphere.com/paper/1705.07581/full.md

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Source: https://tomesphere.com/paper/1705.07581