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|a dc
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|a Cappallo, Roger J.
|e author
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|a Haystack Observatory
|e contributor
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|a MIT Kavli Institute for Astrophysics and Space Research
|e contributor
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|a Cappallo, Roger J.
|e contributor
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|a Corey, Brian E.
|e contributor
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|a Coster, Anthea J.
|e contributor
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|a Erickson, Philip J.
|e contributor
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|a Goeke, Robert F.
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|a Hewitt, Jacqueline N.
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|a Kincaid, Barton B.
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|a Kratzenberg, Eric W.
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|a Lonsdale, Colin John
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|a Matthews, Lynn D.
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|a McWhirter, Stephen R.
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|a Morgan, Edward H.
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|a Remillard, Ronald Alan
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|a Rogers, Alan E. E.
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|a Salah, Joseph E.
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|a Whitney, Alan R.
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|a Williams, Christopher Leigh
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|a Corey, Brian E.
|e author
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|a Coster, Anthea J.
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|a Erickson, Philip J.
|e author
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|a Goeke, Robert F.
|e author
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|a Hewitt, Jacqueline N.
|e author
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|a Kincaid, Barton B.
|e author
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| 700 |
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|a Kratzenberg, Eric W.
|e author
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|a Lonsdale, Colin John
|e author
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| 700 |
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|a Matthews, Lynn D.
|e author
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| 700 |
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|a McWhirter, Stephen R.
|e author
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|a Morgan, Edward H.
|e author
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| 700 |
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|a Remillard, Ronald Alan
|e author
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| 700 |
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|a Rogers, Alan E. E.
|e author
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|a Salah, Joseph E.
|e author
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|a Whitney, Alan R.
|e author
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|a Williams, Christopher Leigh
|e author
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|a Science with the Murchison Widefield Array
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| 260 |
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|b CSIRO Publishing,
|c 2014-07-22T13:21:02Z.
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| 856 |
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|z Get fulltext
|u http://hdl.handle.net/1721.1/88454
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|a 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 arcminute angular resolution and high survey efficiency. The telescope will enable new advances along four key science themes, including searching for redshifted 21-cm emission from the EoR in the early Universe; Galactic and extragalactic all-sky southern hemisphere surveys; time-domain astrophysics; and solar, heliospheric, and ionospheric science and space weather. The Murchison Widefield Array is located in Western Australia at the site of the planned Square Kilometre Array (SKA) low-band telescope and is the only low-frequency SKA precursor facility. In this paper, we review the performance properties of the Murchison Widefield Array and describe its primary scientific objectives.
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|a National Science Foundation (U.S.) (Grant AST-0457585)
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|a National Science Foundation (U.S.) (Grant PHY-0835713)
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|a National Science Foundation (U.S.) (Grant CAREER-0847753)
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|a National Science Foundation (U.S.) (Grant AST-0908884)
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|a United States. Air Force Office of Scientific Research (Grant FA9550-0510247)
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|a Smithsonian Astrophysical Observatory
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|a MIT School of Science
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|a en_US
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|a Article
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|t Publications of the Astronomical Society of Australia
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