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News and Updates

>> 2014-B Observing Proposals are due April 18. Up to 1600 hours of observing time will be awarded. Details are provided in the 2014-B Call for Proposals and the recent Announcement of Opportunity.

>> Mark your calenders: The next MWA Project Science Meeting will be at the Raman Research Institute on 23-25 June 2014.

>> Lead author Dr. Martin Bell (Sydney) and the MWA Team have a new publiction in MNRAS on: A survey for transients and variables with the Murchison Widefield Array 32-tile prototype at 154 MHz (2014)

>> Observers did you know... You can check out the current weather and forecasts for the MWA site.

  • Outrigger tile about 1.5km from the core of the array, with a view of the breakaway behind it. Credit: Natasha Hurley-Walker
  • 28 April 2013: Early look at a test drift scan while commissioning the MWA. Credit: Andre Offringa and MWA Science Commissioning Team
  • Silhouette of an individual dipole. Credit: Natasha Hurley-Walker
  • 12 April 2013: First image from the full MWA! Credit: MWA Science Commissioning Team
  • Image of the nearby radio galaxy Cen A acquired by the MWA development system. Credit: Ben McKinley

The Telescope

The Murchison Widefi eld Array (MWA) is a low-frequency radio telescope operating between 80 and 300 MHz. It is located at the Murchison Radio-astronomy Observatory (MRO) in Western Australia, the planned site of the future Square Kilometre Array (SKA) lowband telescope, and is one of three telescopes designated as a Precursor for the SKA. The MWA has been developed by an international collaboration, including partners from Australia, India, New Zealand, and the United States. It is entering final construction and will be fully operational beginning in 2013. Read more about the telescope...

The Science

The MWA will perform large surveys of the entire Southern Hemisphere sky and acquire deep observations on targeted regions. It will enable astronomers to pursue four key science objectives. The primary endeavor is the hunt for intergalactic hydrogen gas that surrounded early galaxies during the cosmological epoch of reionization. The MWA will also provide new insights into our Milky Way galaxy and its magnetic field, pulsing and exploding stellar objects, and the science of space weather that connects our Sun to the environment here on Earth. Read more about MWA science...