The Murchison Widefield Array: The Square Kilometre Array Precursor at Low Radio Frequencies

• Main Authors: Goeke, Robert F. (Contributor), Lonsdale, Colin John (Contributor), Cappallo, Roger J. (Contributor), Corey, Brian E. (Contributor), Hewitt, Jacqueline N. (Contributor), Kincaid, Barton B. (Contributor), Kratzenberg, Eric W. (Contributor), McWhirter, Stephen R. (Contributor), Morgan, Edward H. (Contributor), Remillard, Ronald Alan (Contributor), Rogers, Alan E. E. (Contributor), Salah, J. E. (Contributor), Whitney, Alan R. (Contributor), Williams, Christopher Leigh (Contributor)
• Other Authors: Haystack Observatory (Contributor), MIT Kavli Institute for Astrophysics and Space Research (Contributor)
• Format: Article
• Language: English
• Published: CSIRO Publishing, 2014-07-22T14:13:51Z.
• Subjects: Article
• Online Access: Get fulltext

 The Murchison Widefield Array (MWA) is one of three Square Kilometre Array Precursor telescopes and is located at the Murchison Radio-astronomy Observatory in the Murchison Shire of the mid-west of Western Australia, a location chosen for its extremely low levels of radio frequency interference. The MWA operates at low radio frequencies, 80-300 MHz, with a processed bandwidth of 30.72 MHz for both linear polarisations, and consists of 128 aperture arrays (known as tiles) distributed over a ~3-km diameter area. Novel hybrid hardware/software correlation and a real-time imaging and calibration systems comprise the MWA signal processing backend. In this paper, the as-built MWA is described both at a system and sub-system level, the expected performance of the array is presented, and the science goals of the instrument are summarised.