M
Mervyn J. Lynch
Researcher at Curtin University
Publications - 104
Citations - 8160
Mervyn J. Lynch is an academic researcher from Curtin University. The author has contributed to research in topics: Murchison Widefield Array & Reionization. The author has an hindex of 39, co-authored 103 publications receiving 7394 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
wsclean: an implementation of a fast, generic wide-field imager for radio astronomy
A. R. Offringa,Benjamin McKinley,Natasha Hurley-Walker,Frank H. Briggs,Randall B. Wayth,Randall B. Wayth,David L. Kaplan,Martin Bell,Martin Bell,Lu Feng,Abraham R. Neben,J. D. Hughes,J. Rhee,Tara Murphy,Tara Murphy,N. D. R. Bhat,Gianni Bernardi,Judd D. Bowman,Roger J. Cappallo,Brian E. Corey,Avinash A. Deshpande,David Emrich,Aaron Ewall-Wice,Bryan Gaensler,Bryan Gaensler,Robert F. Goeke,Lincoln J. Greenhill,Bryna J. Hazelton,Luke Hindson,Melanie Johnston-Hollitt,Daniel C. Jacobs,Justin C. Kasper,Justin C. Kasper,Eric Kratzenberg,Emil Lenc,Emil Lenc,Colin J. Lonsdale,Mervyn J. Lynch,Stephen R. McWhirter,Daniel A. Mitchell,Daniel A. Mitchell,Miguel F. Morales,Edward H. Morgan,Nadia Kudryavtseva,Divya Oberoi,Stephen M. Ord,Stephen M. Ord,Bartosz Pindor,Pietro Procopio,Thiagaraj Prabu,J. Riding,D. A. Roshi,N. Udaya Shankar,K. S. Srivani,Ravi Subrahmanyan,Ravi Subrahmanyan,Steven Tingay,Steven Tingay,Mark Waterson,Mark Waterson,Rachel L. Webster,Rachel L. Webster,Alan R. Whitney,Andrew Williams,Christopher L. Williams +64 more
TL;DR: In this article, the authors present a wide-field interferometric imager that uses the w-stacking algorithm and can make use of the W-snapshot algorithm, which is an order of magnitude faster than w-projection, as well as being capable of full-sky imaging at full resolution with correct polarization correction.
Journal ArticleDOI
The precision array for probing the epoch of re-ionization: eight station results
Aaron R. Parsons,Aaron R. Parsons,Donald C. Backer,Griffin Foster,Melvyn Wright,Richard F. Bradley,Richard F. Bradley,Nicole E. Gugliucci,Chaitali R. Parashare,Erin E. Benoit,James E. Aguirre,Daniel C. Jacobs,Chris Carilli,David Herne,Mervyn J. Lynch,Jason Manley,Dan Werthimer +16 more
TL;DR: The Precision Array for Probing the Epoch of Re-ionization (PAPER) as mentioned in this paper was developed to detect 21 cm emission from the early universe, when the first stars and galaxies were forming.
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.