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    The path to the low frequency Square Kilometre Array in Australia

    Access Status
    Fulltext not available
    Authors
    Tingay, Steven
    Hall, Peter
    Date
    2012
    Type
    Journal Article
    
    Metadata
    Show full item record
    Citation
    Tingay, S. and Hall, P. 2012. The path to the low frequency Square Kilometre Array in Australia. Australian Physics. 49 (6): pp. 174-178.
    Source Title
    Australian Physics
    Additional URLs
    http://astronomy.curtin.edu.au/local/docs/SKA.pdf
    ISSN
    1036-3831
    School
    Curtin Institute of Radio Astronomy (Physics)
    URI
    http://hdl.handle.net/20.500.11937/34481
    Collection
    • Curtin Research Publications
    Abstract

    The Square Kilometre Array (SKA) is a planned next-generation radio telescope to be constructed at two locations, in Western Australia and Southern Africa, utilising a range of antenna technologies to cover the radio frequency range required to satisfy its science goals. The SKA pushes the boundaries of physics and engineering on a number of fronts simultaneously and is thus a very ambitious project with innovation at its heart. In this article we consider the component of the SKA to be built in Western Australia in full scope, a survey telescope designed for very early Universe cosmology, operating at low radio frequencies. The path to the low frequency SKA in Australia involves precursor instrumentation, SKA pre-construction activities, and the deployment of the final instrument in two phases over approximately the next decade.

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