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    The low frequency receivers for SKA 1-low: Design and verification

    Access Status
    Fulltext not available
    Authors
    Benthem, P.
    Gerbers, M.
    De Vaate, J.
    Wynholds, S.
    Bast, J.
    Booler, T.
    Colgate, T.
    Crosse, B.
    Emrich, David
    Hall, Peter
    Juswardy, Budi
    Kerniey, D.
    Schlagenhaufer, Franz
    Sokolowski, Marcin
    Sutinjo, Adrian
    Ung, D.
    Wayth, Randall
    Williams, Andrew
    Alderighi, M.
    Bolli, P.
    Comoretto, G.
    Mattana, A.
    Monari, J.
    Naldi, G.
    Perini, F.
    Pupillo, G.
    Rusticelli, S.
    Schiaffmo, M.
    Schilliro, F.
    Aminei, A.
    Chiello, R.
    Jones, M.
    Baker, J.
    Bennett, R.
    Halsall, R.
    Kaligeridou, G.
    Roberts, M.
    Schnetler, H.
    Abraham, J.
    De Lera Acedo, E.
    Faulkner, A.
    Razavi-Ghods, N.
    Cutajar, D.
    Demarco, A.
    Magro, A.
    Adami, K.
    Date
    2017
    Type
    Conference Paper
    
    Metadata
    Show full item record
    Citation
    Benthem, P. and Gerbers, M. and De Vaate, J. and Wynholds, S. and Bast, J. and Booler, T. and Colgate, T. et al. 2017. The low frequency receivers for SKA 1-low: Design and verification, 2017 XXXIInd General Assembly and Scientific Symposium of the International Union of Radio Science (URSI GASS 2017), pp. 1-4.
    Source Title
    2017 32nd General Assembly and Scientific Symposium of the International Union of Radio Science, URSI GASS 2017
    Source Conference
    2017 XXXIInd General Assembly and Scientific Symposium of the International Union of Radio Science (URSI GASS 2017)
    DOI
    10.23919/URSIGASS.2017.8104992
    ISBN
    9789082598704
    School
    Curtin Institute of Radio Astronomy (Engineering)
    URI
    http://hdl.handle.net/20.500.11937/67896
    Collection
    • Curtin Research Publications
    Abstract

    © 2017 URSI. The initial phase of the Square Kilometre Array (SKA) [1] is represented by a -10% instrument and construction should start in 2018. SKA 1-Low, a sparse Aperture Array (AA) covering the frequency range 50 to 350 MHz, will be part of this. This instrument will consist of 512 stations, each hosting 256 antennas creating a total of 131,072 antennas. A first verification system towards SKA 1-Low, Aperture Array Verification System 1 (AAVSl), is being deployed and validated in 2017.

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