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ASKAP Technologies

The first Phased Array Feed installed on an ASKAP antenna at the Murchison Radio-astronomy Observatory. Image courtesy of DIISR.

ASKAP is designed to be a high speed survey instrument with high dynamic range. This requires an extremely wide field-of-view interferometer with Phased Array Feeds (PAFs) consisting of 188 elements in each of two polarisations as the focal plane detectors.

The specification for ASKAP is:

Technological Goals

To achieve the ASKAP specification, the project's technological goals are to develop:

Opportunities for Industry

Information on opportunities for industry to be involved in the development of ASKAP can be found on the industry page.

Further Information


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