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

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.
National Science Foundation (U.S.) (Grant AST CAREER-0847753)
National Science Foundation (U.S.) (Grant AST-0457585)
National Science Foundation (U.S.) (Grant AST-0908884)
National Science Foundation (U.S.) (Grant PHY-0835713)
United States. Air Force Office of Scientific Research (Grant FA9550-0510247)
Smithsonian Astrophysical Observatory
MIT School of Science