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A fast radio burst with frequency-dependent polarization detected during Breakthrough Listen observations

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posted on 2024-08-06, 12:02 authored by Daniel Price, G. Foster, M. Geyer, W. Van Straten, V. Gajjar, G. Hellbourg, A. Karastergiou, E. F. Keane, A. P.V. Siemion, I. Arcavi, R. Bhat, M. Caleb, S. W. Chang, S. Croft, D. Deboer, I. De Pater, J. Drew, J. E. Enriquez, W. Farah, N. Gizani, J. A. Green, H. Isaacson, J. Hickish, A. Jameson, M. Lebofsky, D. H.E. Macmahon, Anais MollerAnais Moller, C. A. Onken, E. Petroff, D. Werthimer, C. Wolf, S. P. Worden, Y. G. Zhang
Here, we report on the detection and verification of fast radio burst FRB 180301, which occurred on UTC 2018 March 1 during the Breakthrough Listen observations with the Parkes telescope. Full-polarization voltage data of the detection were captured -a first for non-repeating FRBs - allowing for coherent de-dispersion and additional verification tests. The coherently de-dispersed dynamic spectrum of FRB 180301 shows complex, polarized frequency structure over a small fractional bandwidth. As FRB 180301 was detected close to the geosynchronous satellite band during a time of known 1-2 GHz satellite transmissions, we consider whether the burst was due to radio interference emitted or reflected from an orbiting object. Based on the pre-ponderance of our verification tests, we cannot conclusively determine FRB 180301 to be either astrophysical or anthropogenic in origin.

Funding

Mapping the universe with the Panoramic Survey Telescope and Rapid Response System (PanSTARRS)

Australian Research Council

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CE110001020:ARC

ARC Centre of Excellence for Gravitational Wave Discovery

Australian Research Council

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ISSN

1365-2966

Journal title

Monthly Notices of the Royal Astronomical Society

Volume

486

Issue

3

Pagination

10 pp

Publisher

Oxford University Press (OUP)

Copyright statement

This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society. Copyright © 2019 The Authors. Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.

Language

eng

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