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A single fast radio burst localized to a massive galaxy at cosmological distance

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posted on 2024-08-06, 12:01 authored by K. W. Bannister, Adam DellerAdam Deller, C. Phillips, J. P. Macquart, J. X. Prochaska, N. Tejos, S. D. Ryder, E. M. Sadler, Ryan ShannonRyan Shannon, S. Simha, C. K. Day, M. McQuinn, F. O. North-Hickey, S. Bhandari, W. R. Arcus, V. N. Bennert, J. Burchett, M. Bouwhuis, R. Dodson, R. D. Ekers, W. Farah, Christopher FlynnChristopher Flynn, C. W. James, M. Kerr, E. Lenc, E. K. Mahony, J. O'Meara, Stefan Oslowski, H. Qiu, T. Treu, V. U, T. J. Bateman, D. C.J. Bock, R. J. Bolton, A. Brown, J. D. Bunton, A. P. Chippendale, F. R. Cooray, T. Cornwell, N. Gupta, D. B. Hayman, M. Kesteven, B. S. Koribalski, A. Macleod, N. M. McClure-Griffiths, S. Neuhold, R. P. Norris, M. A. Pilawa, R. Y. Qiao, J. Reynolds, D. N. Roxby, T. W. Shimwell, M. A. Voronkov, C. D. Wilson
Fast Radio Bursts (FRBs) are brief radio emissions from distant astronomical sources. Some are known to repeat, but most are single bursts. Non-repeating FRB observations have had insufficient positional accuracy to localize them to an individual host galaxy. We report the interferometric localization of the single pulse FRB 180924 to a position 4 kpc from the center of a luminous galaxy at redshift 0.3214. The burst has not been observed to repeat. The properties of the burst and its host are markedly different from the only other accurately localized FRB source. The integrated electron column density along the line of sight closely matches models of the intergalactic medium, indicating that some FRBs are clean probes of the baryonic component of the cosmic web.

Funding

Weighing the Universe using fast radio bursts

Australian Research Council

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Pinpointing the hosts of Fast Radio Bursts with UTMOST-2D

Australian Research Council

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Exascale astronomy: real-time analysis of the transient radio universe

Australian Research Council

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ARC Centre of Excellence for Gravitational Wave Discovery

Australian Research Council

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History

Available versions

PDF (Accepted manuscript)

ISSN

1095-9203

Journal title

Science

Volume

365

Issue

6453

Pagination

5 pp

Publisher

American Association for the Advancement of Science (AAAS)

Copyright statement

Copyright © 2019 the authors. This is the author’s version of the work. It is posted here by permission of the AAAS for personal use, not for redistribution. The definitive version was published in Science, on 09 Aug 2019, Vol. 365, Issue 6453, DOI: 10.1126/science.aaw5903.

Notes

Many additional authors listed at publishers page

Language

eng

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