A single fast radio burst localized to a massive galaxy at cosmological distance-Reference-Cited by-同舟云学术

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

Published:2019-08-09 Issue:6453 Volume:365 Page:565-570
ISSN:0036-8075
Container-title:Science
language:en
Short-container-title:Science

Author:

Bannister K. W.¹^ORCID,Deller A. T.²^ORCID,Phillips C.¹^ORCID,Macquart J.-P.³^ORCID,Prochaska J. X.⁴⁵^ORCID,Tejos N.⁶^ORCID,Ryder S. D.⁷^ORCID,Sadler E. M.¹⁸^ORCID,Shannon R. M.²^ORCID,Simha S.⁴^ORCID,Day C. K.²^ORCID,McQuinn M.⁹^ORCID,North-Hickey F. O.³^ORCID,Bhandari S.¹^ORCID,Arcus W. R.³,Bennert V. N.¹⁰,Burchett J.⁶^ORCID,Bouwhuis M.¹¹¹^ORCID,Dodson R.¹²,Ekers R. D.¹³^ORCID,Farah W.²^ORCID,Flynn C.²,James C. W.³^ORCID,Kerr M.¹³^ORCID,Lenc E.¹^ORCID,Mahony E. K.¹^ORCID,O’Meara J.¹⁴^ORCID,Osłowski S.²^ORCID,Qiu H.¹⁸^ORCID,Treu T.¹⁵^ORCID,U V.¹⁶^ORCID,Bateman T. J.⁸^ORCID,Bock D. C.-J.¹^ORCID,Bolton R. J.¹^ORCID,Brown A.¹,Bunton J. D.¹^ORCID,Chippendale A. P.¹^ORCID,Cooray F. R.¹,Cornwell T.¹⁷^ORCID,Gupta N.¹⁸^ORCID,Hayman D. B.¹^ORCID,Kesteven M.¹,Koribalski B. S.¹^ORCID,MacLeod A.¹^ORCID,McClure-Griffiths N. M.¹⁹^ORCID,Neuhold S.¹,Norris R. P.¹²⁰^ORCID,Pilawa M. A.¹,Qiao R.-Y.¹,Reynolds J.¹^ORCID,Roxby D. N.¹,Shimwell T. W.²¹^ORCID,Voronkov M. A.¹^ORCID,Wilson C. D.¹^ORCID

Affiliation:

1. Commonwealth Science and Industrial Research Organisation, Australia Telescope National Facility, P.O. Box 76, Epping, NSW 1710, Australia.

2. Centre for Astrophysics and Supercomputing, Swinburne University of Technology, Hawthorn, VIC 3122, Australia.

3. International Centre for Radio Astronomy Research, Curtin University, Bentley, WA 6102, Australia.

4. University of California Observatories–Lick Observatory, University of California, Santa Cruz, CA 95064, USA.

5. Kavli Institute for the Physics and Mathematics of the Universe, 5-1-5 Kashiwanoha, Kashiwa 277-8583, Japan.

6. Instituto de Física, Pontificia Universidad Católica de Valparaíso, Casilla 4059, Valparaíso, Chile.

7. Department of Physics and Astronomy, Macquarie University, North Ryde, NSW 2109, Australia.

8. Sydney Institute for Astronomy, School of Physics, University of Sydney, Sydney, NSW 2006, Australia.

9. Astronomy Department, University of Washington, Seattle, WA 98195, USA.

10. Physics Department, California Polytechnic State University, San Luis Obispo, CA 93407, USA.

11. Nikhef, Science Park, Amsterdam, Netherlands.

12. International Centre for Radio Astronomy Research, University of Western Australia, Crawley, Perth, WA 6009, Australia.

13. Space Science Division, Naval Research Laboratory, Washington, DC 20375, USA.

14. W. M. Keck Observatory, Waimea, HI 96743, USA.

15. Department of Physics and Astronomy, University of California, Los Angeles, CA 90095, USA.

16. Department of Physics and Astronomy, University of California, Irvine, CA 92697, USA.

17. Tim Cornwell Consulting, 17 Elgan Crescent, Sandbach CW11 1LD, UK.

18. Inter-University Centre for Astronomy and Astrophysics, Post Bag 4, Ganeshkhind, Pune 411 007, India.

19. Research School of Astronomy and Astrophysics, Australian National University, Canberra, ACT 2611, Australia.

20. Western Sydney University, Locked Bag 1797, Penrith South, NSW 2751, Australia.

21. ASTRON, Netherlands Institute for Radio Astronomy, Postbus 2, 7990 AA Dwingeloo, Netherlands.

Abstract

Pinpointing a single fast radio burst Fast radio bursts (FRBs) are flashes of radio emission from distant astronomical sources. Two FRBs are known to have repeated, but most last just a few milliseconds and are never seen again. Most telescopes that are sensitive to single FRBs have poor angular resolutions, so the FRB host galaxies remain unknown. Bannister et al. used a dedicated observing mode on a radio interferometer to detect and localize the nonrepeating FRB 180924, then followed up with optical telescope observations (see the Perspective by Petroff). They found that the FRB came from a medium-sized galaxy at a cosmological distance. Localizing FRBs will help determine their causes and allow them to be used as cosmological probes. Science , this issue p. 565 ; see also p. 546

Funder

Australian Research Council

Publisher

American Association for the Advancement of Science (AAAS)

Subject

Multidisciplinary

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2. THE BARYON CENSUS IN A MULTIPHASE INTERGALACTIC MEDIUM: 30% OF THE BARYONS MAY STILL BE MISSING

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