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

DOI DOI DOI DOI DOI ほか6件をすべて表示 一部だけ表示 被引用文献13件 オープンアクセス
  • K. W. Bannister
    Commonwealth Science and Industrial Research Organisation, Australia Telescope National Facility, P.O. Box 76, Epping, NSW 1710, Australia.
  • A. T. Deller
    Centre for Astrophysics and Supercomputing, Swinburne University of Technology, Hawthorn, VIC 3122, Australia.
  • C. Phillips
    Commonwealth Science and Industrial Research Organisation, Australia Telescope National Facility, P.O. Box 76, Epping, NSW 1710, Australia.
  • J.-P. Macquart
    International Centre for Radio Astronomy Research, Curtin University, Bentley, WA 6102, Australia.
  • J. X. Prochaska
    University of California Observatories–Lick Observatory, University of California, Santa Cruz, CA 95064, USA.
  • N. Tejos
    Instituto de Física, Pontificia Universidad Católica de Valparaíso, Casilla 4059, Valparaíso, Chile.
  • S. D. Ryder
    Department of Physics and Astronomy, Macquarie University, North Ryde, NSW 2109, Australia.
  • E. M. Sadler
    Commonwealth Science and Industrial Research Organisation, Australia Telescope National Facility, P.O. Box 76, Epping, NSW 1710, Australia.
  • R. M. Shannon
    Centre for Astrophysics and Supercomputing, Swinburne University of Technology, Hawthorn, VIC 3122, Australia.
  • S. Simha
    University of California Observatories–Lick Observatory, University of California, Santa Cruz, CA 95064, USA.
  • C. K. Day
    Centre for Astrophysics and Supercomputing, Swinburne University of Technology, Hawthorn, VIC 3122, Australia.
  • M. McQuinn
    Astronomy Department, University of Washington, Seattle, WA 98195, USA.
  • F. O. North-Hickey
    International Centre for Radio Astronomy Research, Curtin University, Bentley, WA 6102, Australia.
  • S. Bhandari
    Commonwealth Science and Industrial Research Organisation, Australia Telescope National Facility, P.O. Box 76, Epping, NSW 1710, Australia.
  • W. R. Arcus
    International Centre for Radio Astronomy Research, Curtin University, Bentley, WA 6102, Australia.
  • V. N. Bennert
    Physics Department, California Polytechnic State University, San Luis Obispo, CA 93407, USA.
  • J. Burchett
    Instituto de Física, Pontificia Universidad Católica de Valparaíso, Casilla 4059, Valparaíso, Chile.
  • M. Bouwhuis
    Commonwealth Science and Industrial Research Organisation, Australia Telescope National Facility, P.O. Box 76, Epping, NSW 1710, Australia.
  • R. Dodson
    International Centre for Radio Astronomy Research, University of Western Australia, Crawley, Perth, WA 6009, Australia.
  • R. D. Ekers
    Commonwealth Science and Industrial Research Organisation, Australia Telescope National Facility, P.O. Box 76, Epping, NSW 1710, Australia.
  • W. Farah
    Centre for Astrophysics and Supercomputing, Swinburne University of Technology, Hawthorn, VIC 3122, Australia.
  • C. Flynn
    Centre for Astrophysics and Supercomputing, Swinburne University of Technology, Hawthorn, VIC 3122, Australia.
  • C. W. James
    International Centre for Radio Astronomy Research, Curtin University, Bentley, WA 6102, Australia.
  • M. Kerr
    Space Science Division, Naval Research Laboratory, Washington, DC 20375, USA.
  • E. Lenc
    Commonwealth Science and Industrial Research Organisation, Australia Telescope National Facility, P.O. Box 76, Epping, NSW 1710, Australia.
  • E. K. Mahony
    Commonwealth Science and Industrial Research Organisation, Australia Telescope National Facility, P.O. Box 76, Epping, NSW 1710, Australia.
  • J. O’Meara
    W. M. Keck Observatory, Waimea, HI 96743, USA.
  • S. Osłowski
    Centre for Astrophysics and Supercomputing, Swinburne University of Technology, Hawthorn, VIC 3122, Australia.
  • H. Qiu
    Commonwealth Science and Industrial Research Organisation, Australia Telescope National Facility, P.O. Box 76, Epping, NSW 1710, Australia.
  • T. Treu
    Department of Physics and Astronomy, University of California, Los Angeles, CA 90095, USA.
  • V. U
    Department of Physics and Astronomy, University of California, Irvine, CA 92697, USA.
  • T. J. Bateman
    Sydney Institute for Astronomy, School of Physics, University of Sydney, Sydney, NSW 2006, Australia.
  • D. C.-J. Bock
    Commonwealth Science and Industrial Research Organisation, Australia Telescope National Facility, P.O. Box 76, Epping, NSW 1710, Australia.
  • R. J. Bolton
    Commonwealth Science and Industrial Research Organisation, Australia Telescope National Facility, P.O. Box 76, Epping, NSW 1710, Australia.
  • A. Brown
    Commonwealth Science and Industrial Research Organisation, Australia Telescope National Facility, P.O. Box 76, Epping, NSW 1710, Australia.
  • J. D. Bunton
    Commonwealth Science and Industrial Research Organisation, Australia Telescope National Facility, P.O. Box 76, Epping, NSW 1710, Australia.
  • A. P. Chippendale
    Commonwealth Science and Industrial Research Organisation, Australia Telescope National Facility, P.O. Box 76, Epping, NSW 1710, Australia.
  • F. R. Cooray
    Commonwealth Science and Industrial Research Organisation, Australia Telescope National Facility, P.O. Box 76, Epping, NSW 1710, Australia.
  • T. Cornwell
    Tim Cornwell Consulting, 17 Elgan Crescent, Sandbach CW11 1LD, UK.
  • N. Gupta
    Inter-University Centre for Astronomy and Astrophysics, Post Bag 4, Ganeshkhind, Pune 411 007, India.
  • D. B. Hayman
    Commonwealth Science and Industrial Research Organisation, Australia Telescope National Facility, P.O. Box 76, Epping, NSW 1710, Australia.
  • M. Kesteven
    Commonwealth Science and Industrial Research Organisation, Australia Telescope National Facility, P.O. Box 76, Epping, NSW 1710, Australia.
  • B. S. Koribalski
    Commonwealth Science and Industrial Research Organisation, Australia Telescope National Facility, P.O. Box 76, Epping, NSW 1710, Australia.
  • A. MacLeod
    Commonwealth Science and Industrial Research Organisation, Australia Telescope National Facility, P.O. Box 76, Epping, NSW 1710, Australia.
  • N. M. McClure-Griffiths
    Research School of Astronomy and Astrophysics, Australian National University, Canberra, ACT 2611, Australia.
  • S. Neuhold
    Commonwealth Science and Industrial Research Organisation, Australia Telescope National Facility, P.O. Box 76, Epping, NSW 1710, Australia.
  • R. P. Norris
    Commonwealth Science and Industrial Research Organisation, Australia Telescope National Facility, P.O. Box 76, Epping, NSW 1710, Australia.
  • M. A. Pilawa
    Commonwealth Science and Industrial Research Organisation, Australia Telescope National Facility, P.O. Box 76, Epping, NSW 1710, Australia.
  • R.-Y. Qiao
    Commonwealth Science and Industrial Research Organisation, Australia Telescope National Facility, P.O. Box 76, Epping, NSW 1710, Australia.
  • J. Reynolds
    Commonwealth Science and Industrial Research Organisation, Australia Telescope National Facility, P.O. Box 76, Epping, NSW 1710, Australia.
  • D. N. Roxby
    Commonwealth Science and Industrial Research Organisation, Australia Telescope National Facility, P.O. Box 76, Epping, NSW 1710, Australia.
  • T. W. Shimwell
    ASTRON, Netherlands Institute for Radio Astronomy, Postbus 2, 7990 AA Dwingeloo, Netherlands.
  • M. A. Voronkov
    Commonwealth Science and Industrial Research Organisation, Australia Telescope National Facility, P.O. Box 76, Epping, NSW 1710, Australia.
  • C. D. Wilson
    Commonwealth Science and Industrial Research Organisation, Australia Telescope National Facility, P.O. Box 76, Epping, NSW 1710, Australia.
  • Swinburne University of Technology
  • School of Computing, Engineering and Mathematics (Host institution)

書誌事項

公開日
2019-08-09
DOI
  • 10.1126/science.aaw5903
  • 10.25916/sut.26250932.v1
  • 10.25916/sut.26250932.v2
  • 10.48550/arxiv.1906.11476
  • 10.25916/sut.26250932
公開者
American Association for the Advancement of Science (AAAS)

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説明

<jats:title>Pinpointing a single fast radio burst</jats:title> <jats:p> 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 <jats:italic>et al.</jats:italic> 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. </jats:p> <jats:p> <jats:italic>Science</jats:italic> , this issue p. <jats:related-article xmlns:xlink="http://www.w3.org/1999/xlink" ext-link-type="doi" issue="6453" page="565" related-article-type="in-this-issue" vol="365" xlink:href="10.1126/science.aaw5903">565</jats:related-article> ; see also p. <jats:related-article xmlns:xlink="http://www.w3.org/1999/xlink" ext-link-type="doi" issue="6453" page="546" related-article-type="in-this-issue" vol="365" xlink:href="10.1126/science.aay4330">546</jats:related-article> </jats:p>

収録刊行物

  • Science

    Science 365 (6453), 565-570, 2019-08-09

    American Association for the Advancement of Science (AAAS)

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