B
B. B. Kincaid
Researcher at Massachusetts Institute of Technology
Publications - 32
Citations - 4544
B. B. Kincaid is an academic researcher from Massachusetts Institute of Technology. The author has contributed to research in topics: Murchison Widefield Array & Reionization. The author has an hindex of 21, co-authored 32 publications receiving 4295 citations.
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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
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.
Journal ArticleDOI
The Murchison Widefield Array: Design Overview
Colin J. Lonsdale,Roger J. Cappallo,Miguel F. Morales,Frank H. Briggs,L. Benkevitch,Judd D. Bowman,John D. Bunton,Steven Burns,Brian E. Corey,Ludi deSouza,Sheperd S. Doeleman,Mark Derome,Avinash A. Deshpande,M. R. Gopalakrishna,Lincoln J. Greenhill,David Herne,Jacqueline N. Hewitt,P. A. Kamini,Justin C. Kasper,B. B. Kincaid,Jonathan Kocz,Errol Kowald,Eric Kratzenberg,Deepak Kumar,Mervyn J. Lynch,S. Madhavi,Michael Matejek,Daniel A. Mitchell,Edward H. Morgan,Divya Oberoi,Steven Ord,Joseph Pathikulangara,Thiagaraj Prabu,Alan E. E. Rogers,A. Roshi,Joseph E. Salah,Robert J. Sault,N. Udaya Shankar,K. S. Srivani,Jamie Stevens,Steven Tingay,Annino Vaccarella,Mark Waterson,Randall B. Wayth,Rachel L. Webster,Alan R. Whitney,Andrew Williams,Christopher L. Williams +47 more
TL;DR: The Murchison Widefield Array (MWA) as discussed by the authors is a dipole-based aperture array synthesis telescope designed to operate in the 80-300 MHz frequency range and is capable of a wide range of science investigations, but is initially focused on three key science projects.