J
John D. Bunton
Researcher at Commonwealth Scientific and Industrial Research Organisation
Publications - 169
Citations - 9083
John D. Bunton is an academic researcher from Commonwealth Scientific and Industrial Research Organisation. The author has contributed to research in topics: Murchison Widefield Array & Radio telescope. The author has an hindex of 40, co-authored 165 publications receiving 8130 citations. Previous affiliations of John D. Bunton include Australia Telescope National Facility & ASTRON.
Papers
More filters
Journal ArticleDOI
The Murchison widefield array: The square kilometre array precursor at low radio frequencies
Steven Tingay,Robert F. Goeke,Judd D. Bowman,David Emrich,Stephen M. Ord,Daniel A. Mitchell,Miguel F. Morales,T. Booler,Brian Crosse,Randall B. Wayth,Colin J. Lonsdale,S. E. Tremblay,D. Pallot,T. Colegate,Andreas Wicenec,Nadia Kudryavtseva,W. Arcus,David G. Barnes,Gianni Bernardi,Frank H. Briggs,S. Burns,John D. Bunton,Roger J. Cappallo,Brian E. Corey,Avinash A. Deshpande,Ludi deSouza,Bryan Gaensler,Lincoln J. Greenhill,Peter J. Hall,Bryna J. Hazelton,David Herne,Jacqueline N. Hewitt,Melanie Johnston-Hollitt,David L. Kaplan,Justin C. Kasper,B. B. Kincaid,R. Koenig,Eric Kratzenberg,Mervyn J. Lynch,Benjamin McKinley,Stephen R. McWhirter,Edward H. Morgan,Divya Oberoi,Joseph Pathikulangara,Thiagaraj Prabu,Ron Remillard,Alan E. E. Rogers,A. Roshi,Joseph E. Salah,Robert J. Sault,N. Udaya-Shankar,F. Schlagenhaufer,K. S. Srivani,Jamie Stevens,Ravi Subrahmanyan,M. Waterson,Rachel L. Webster,Alan R. Whitney,Andrew Williams,Christopher L. Williams,J. S. B. Wyithe +60 more
TL;DR: The Murchison Widefield Array (MWA) as discussed by the authors is one of three Square Kilometre Array Precursor telescopes and is located at the MUR-astronomy Observatory in Western Australia, a location chosen for its extremely low levels of radio frequency interference.
Journal ArticleDOI
The Murchison Widefield Array: the Square Kilometre Array Precursor at low radio frequencies
Steven Tingay,Robert F. Goeke,Judd D. Bowman,David Emrich,Stephen M. Ord,Daniel A. Mitchell,Miguel F. Morales,Tom Booler,Brian Crosse,D. Pallot,Andreas Wicenec,W. Arcus,David G. Barnes,Gianni Bernardi,Frank H. Briggs,S. Burns,John D. Bunton,Roger J. Cappallo,T. Colegate,Brian E. Corey,Avinash A. Deshpande,L. deSouza,Bryan Gaensler,Lincoln J. Greenhill,J. Hall,Bryna J. Hazelton,David Herne,Jacqueline N. Hewitt,Melanie Johnston-Hollitt,David L. Kaplan,Justin C. Kasper,B. B. Kincaid,R. Koenig,Eric Kratzenberg,Colin J. Lonsdale,Mervyn J. Lynch,Benjamin McKinley,Stephen R. McWhirter,Edward H. Morgan,Divya Oberoi,Joseph Pathikulangara,Thiagaraj Prabu,Ron Remillard,Alan E. E. Rogers,A. Roshi,Joseph E. Salah,Robert J. Sault,N. Udaya-Shankar,F. Schlagenhaufer,K. S. Srivani,Jamie Stevens,Ravi Subrahmanyan,S. E. Tremblay,Randall B. Wayth,M. Waterson,Rachel L. Webster,Alan R. Whitney,Andrew Williams,Christopher L. Williams,J. S. B. Wyithe +59 more
TL;DR: The Murchison Widefield Array (MWA) as mentioned in this paper is one of three Square Kilometre Array Precursor telescopes and is located at the MUR-astronomy Observatory in Western Australia, a location chosen for its extremely low levels of radio frequency interference.
Journal ArticleDOI
The Murchison Widefield Array: Design Overview
Colin J. Lonsdale,Roger J. Cappallo,Miguel F. Morales,Miguel F. Morales,Frank H. Briggs,L. Benkevitch,Judd D. Bowman,John D. Bunton,S. Burns,Brian E. Corey,Ludi deSouza,S. Doeleman,Mark Derome,Avinash A. Deshpande,M.R. Gopala,Lincoln J. Greenhill,David Herne,Jacqueline N. Hewitt,P. A. Kamini,Justin C. Kasper,B. B. Kincaid,Jonathon Kocz,E. Kowald,Eric Kratzenberg,Deepak Kumar,Mervyn J. Lynch,S. Madhavi,Michael Matejek,Daniel A. Mitchell,Edward H. Morgan,Divya Oberoi,Stephen M. Ord,Joseph Pathikulangara,Thiagaraj Prabu,Alan E. E. Rogers,A. Roshi,Joseph E. Salah,Robert J. Sault,N. U. Shankar,K. S. Srivani,Jamie Stevens,Steven Tingay,A. Vaccarella,M. Waterson,Randall B. Wayth,Rachel L. Webster,Alan R. Whitney,Andrew Williams,Christopher L. Williams +48 more
TL;DR: The Murchison Widefield Array is a dipole-based aperture array synthesis telescope designed to operate in the 80-300 MHz frequency range, capable of a wide range of science investigations but initially focused on three key science projects: detection and characterization of three-dimensional brightness temperature fluctuations in the 21 cm line of neutral hydrogen during the epoch of reionization.
Journal ArticleDOI
A single fast radio burst localized to a massive galaxy at cosmological distance
Keith W. Bannister,Adam Deller,Chris Phillips,Jean-Pierre Macquart,Jason X. Prochaska,Jason X. Prochaska,Nicolas Tejos,Stuart D. Ryder,Elaine M. Sadler,Elaine M. Sadler,Ryan Shannon,Sunil Simha,Cherie K. Day,Matthew McQuinn,F. O. North-Hickey,Shivani Bhandari,W. Arcus,Vardha N. Bennert,J. N. Burchett,M. Bouwhuis,Richard Dodson,Ron Ekers,Ron Ekers,Wael Farah,Chris Flynn,C. W. James,Matthew Kerr,Emil Lenc,Elizabeth K. Mahony,John M. O'Meara,Stefan Oslowski,Hao Qiu,Hao Qiu,Tommaso Treu,T. Bateman,Douglas C.-J. Bock,R. J. Bolton,Anthony G. A. Brown,John D. Bunton,Aaron Chippendale,F. R. Cooray,Tim J. Cornwell,N. Gupta,Douglas B. Hayman,Michael Kesteven,Bärbel S. Koribalski,A. Macleod,Naomi McClure-Griffiths,S. Neuhold,Ray P. Norris,Ray P. Norris,M. A. Pilawa,R.-Y. Qiao,John Reynolds,Daniel N. Roxby,Timothy W. Shimwell,Maxim Voronkov,Christine D. Wilson +57 more
TL;DR: In this paper, the authors reported the interferometric localization of the single-pulse fast radio burst (FRB 180924) to a position 4 kiloparsecs from the center of a luminous galaxy at redshift 0.3214.
Journal ArticleDOI
Science with the Murchison Widefield Array
Judd D. Bowman,Iver H. Cairns,David L. Kaplan,Tara Murphy,Divya Oberoi,Lister Staveley-Smith,W. Arcus,David G. Barnes,Gianni Bernardi,Frank H. Briggs,Shea Brown,John D. Bunton,Adam J. Burgasser,Roger J. Cappallo,Shami Chatterjee,Brian E. Corey,Anthea J. Coster,Avinash A. Deshpande,L. deSouza,David Emrich,Philip J. Erickson,Robert F. Goeke,Bryan Gaensler,Lincoln J. Greenhill,Lisa Harvey-Smith,Bryna J. Hazelton,David Herne,Jacqueline N. Hewitt,Melanie Johnston-Hollitt,Justin C. Kasper,B. B. Kincaid,R. Koenig,Eric Kratzenberg,Colin J. Lonsdale,Mervyn J. Lynch,Lynn D. Matthews,S. Russell McWhirter,Daniel A. Mitchell,Miguel F. Morales,Edward H. Morgan,Stephen M. Ord,Joseph Pathikulangara,Thiagaraj Prabu,Ronald A. Remillard,Timothy Robishaw,Alan E. E. Rogers,A. Roshi,Joseph E. Salah,Robert J. Sault,N. Udaya Shankar,K. S. Srivani,J. Stevens,Ravi Subrahmanyan,Steven Tingay,Randall B. Wayth,M. Waterson,Rachel L. Webster,Alan R. Whitney,Andrew Williams,Christopher L. Williams,J. Stuart B. Wyithe +60 more
TL;DR: The Murchison Widefield Array (MWA) as discussed by the authors is the first telescope in the southern hemisphere designed specifically to explore the low-frequency astronomical sky between 80 and 300 MHz with arcminute angular resolution and high survey efficiency.