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    First results from AAVS 0.5: A prototype array for next-generation radio astronomy

    193928_193928.pdf (1.057Mb)
    Access Status
    Open access
    Authors
    Hall, Peter
    Sutinjo, Adrian
    de Lera Acedo, E.
    Wayth, Randall
    Razavi-Ghods, N.
    Colegate, Timothy
    Faulkner, A.
    Juswardy, Budi
    Fiorelli, B
    Booler, Tom
    Bij de Vaate, J.
    Waterson, Mark
    Tingay, Steven
    Date
    2013
    Type
    Conference Paper
    
    Metadata
    Show full item record
    Citation
    Hall, P.J. and Sutinjo, A.T. and de Lera Acedo, E. and Wayth, R.B. and Razavi-Ghods, N. and Colegate, T.M. and Faulkner, A.J. and Juswardy, B. and Fiorelli, B. and Booler, T. and Bij de Vaate, J.G. and Waterson, M. and Tingay, S.J. 2013. First results from AAVS 0.5: A prototype array for next-generation radio astronomy, in International Conference on Electromagnetics in Advanced Applications, Sep 9-13 2013, pp. 340-343. Torino, Italy: IEEE.
    Source Title
    International Conference on Electromagnetics in Advanced Applications (ICEAA 2013)
    Source Conference
    International Conference on Electromagnetics in Advanced Applications
    DOI
    10.1109/ICEAA.2013.6632250
    ISBN
    978-1-4673-5705-0
    Remarks

    Copyright © 2013 IEEE. Personal use of this material is permitted. Permission from IEEE must be obtained for all other uses, in any current or future media, including reprinting/republishing this material for advertising or promotional purposes, creating new collective works, for resale or redistribution to servers or lists, or reuse of any copyrighted component of this work in other works.

    URI
    http://hdl.handle.net/20.500.11937/38746
    Collection
    • Curtin Research Publications
    Abstract

    This paper provides an overview of the Aperture Array Verification System 0.5 (AAVS 0.5), co-located and operated in conjunction with the Murchison Widefield Array (MWA) near the Australian SKA core site. AAVS 0.5 is based on log-periodic antennas of a type potentially useful in next-generation low-frequency arrays such as SKA-low. We report on our progress by discussing results obtained thus far as well as test plans for the near future. A number of lessons learned will be presented, demonstrating that hands-on experience constitutes an essential knowledge-base in the pre-construction phase of a radio-telescope such as the SKA.

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