Science with the Murchison Widefield Array

D. Bowman, Judd; Cairns, Iver; L. Kaplan, David; Murphy, Tara; Oberoi, Divya; Staveley-Smith, Lister; Arcus, Wayne; G. Barnes, David; Bernardi, Gianni; H. Briggs, Frank; Brown, Shea; D. Bunton, John; J. Burgasser, Adam; J. Cappallo, Roger; Chatterjee, Shami; E. Corey, Brian; Coster, Anthea; Deshpande, Avinash; deSouza, Ludi; Emrich, David; Erickson, Philip; F. Goeke, Robert; M. Gaensler, B.; J. Greenhill, Lincoln; Harvey-Smith, Lisa; J. Hazelton, Bryna; Herne, David; N. Hewitt, Jacqueline; Johnston-Hollitt, Melanie; C. Kasper, Justin; B. Kincaid, Barton; Koenig, Ronald; Kratzenberg, Eric; J. Lonsdale, Colin; J. Lynch, Mervyn; D. Matthews, Lynn; Russell McWhirter, S.; A. Mitchell, Daniel; F. Morales, Miguel; H. Morgan, Edward; M. Ord, Stephen; Pathikulangara, Joseph; Prabu, Thiagaraj; A. Remillard, Ronald; Robishaw, Timothy; E. E. Rogers, Alan; A. Roshi, Anish; E. Salah, Joseph; J. Sault, Robert; Udaya Shankar, N.; S. Srivani, K.; B. Stevens, Jamie; Subrahmanyan, Ravi; J. Tingay, Steven; B. Wayth, Randall; Waterson, Mark; L. Webster, Rachel; R. Whitney, Alan; J. Williams, Andrew; L. Williams, Christopher; Stuart B. Wyithe, J.

doi:10.1017/pas.2013.009

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Science with the Murchison Widefield Array

Shared by NobleBlocks on Jan 1, 2013 • 12:00 AM UTC

Authors:

Judd D. Bowman

Iver Cairns

David L. Kaplan

Abstract

Abstract Significant new opportunities for astrophysics and cosmology have been identified at low radio frequencies. The Murchison Widefield Array is the first telescope in the southern hemisphere designed specifically to explore the low-frequency astronomical sky between 80 and 300 MHz with arcminu...

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