Flexibility to accommodate a wide range of science cases

The MWA has expanded, with marked improvements in its engineering characteristics increasing the breadth and depth of observable sky. Click on the links below to learn more about the different stages of the telescope.

Phase I

The original 128-tile array, with antennas dispersed in a spiral pattern with a dense core.

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Phase II

An additional 128 tiles create array configurations of compact and extended baselines.

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