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    A digital-receiver for the Murchison Widefield Array

    233237_233237.pdf (947.6Kb)
    Access Status
    Open access
    Authors
    Prabu, T.
    Srivani, K.
    Roshi, D.
    Kamini, P.
    Madhavi, S.
    Emrich, D.
    Crosse, B.
    Williams, A.
    Waterson, M.
    Deshpande, A.
    Shankar, N.
    Subrahmanyan, R.
    Briggs, F.
    Goeke, R.
    Tingay, Steven
    Johnston-Hollitt, M.
    R, G.
    Morgan, E.
    Pathikulangara, J.
    Bunton, J.
    Hampson, G.
    Williams, C.
    Ord, Stephen
    Wayth, Randall
    Kumar, D.
    Morales, M.
    DeSouza, L.
    Kratzenberg, E.
    Pallot, D.
    McWhirter, R.
    Hazelton, B.
    Arcus, W.
    Barnes, D.
    Bernardi, G.
    Booler, T.
    Bowman, J.
    Cappallo, R.
    Corey, B.
    Greenhill, L.
    Herne, D.
    Hewitt, J.
    Kaplan, D.
    Kasper, J.
    Kincaid, B.
    Koenig, R.
    Lonsdale, C.
    Lynch, Mervyn
    Mitchell, D.
    Oberoi, D.
    Remillard, R.
    Rogers, A.
    Salah, J.
    Sault, R.
    Stevens, J.
    Tremblay, S.
    Webster, R.
    Whitney, A.
    Wyithe, S.
    Date
    2015
    Type
    Journal Article
    
    Metadata
    Show full item record
    Citation
    Prabu, T. and Srivani, K. and Roshi, D. and Kamini, P. and Madhavi, S. and Emrich, D. and Crosse, B. et al. 2015. A digital-receiver for the Murchison Widefield Array. Experimental Astronomy. 39 (1): pp. 73-93.
    Source Title
    Experimental Astronomy
    DOI
    10.1007/s10686-015-9444-3
    ISSN
    0922-6435
    School
    Curtin Institute of Radio Astronomy (Physics)
    Remarks

    The final publication is available at Springer via http://doi.org/10.1007/s10686-015-9444-3

    URI
    http://hdl.handle.net/20.500.11937/37271
    Collection
    • Curtin Research Publications
    Abstract

    An FPGA-based digital-receiver has been developed for a low-frequency imaging radio interferometer, the Murchison Widefield Array (MWA). The MWA, located at the Murchison Radio-astronomy Observatory (MRO) in Western Australia, consists of 128 dual-polarized aperture-array elements (tiles) operating between 80 and 300 MHz, with a total processed bandwidth of 30.72 MHz for each polarization. Radio-frequency signals from the tiles are amplified and band limited using analog signal conditioning units; sampled and channelized by digital-receivers. The signals from eight tiles are processed by a single digital-receiver, thus requiring 16 digital-receivers for the MWA. The main function of the digital-receivers is to digitize the broad-band signals from each tile, channelize them to form the sky-band, and transport it through optical fibers to a centrally located correlator for further processing. The digital-receiver firmware also implements functions to measure the signal power, perform power equalization across the band, detect interference-like events, and invoke diagnostic modes. The digital-receiver is controlled by high-level programs running on a single-board-computer. This paper presents the digital-receiver design, implementation, current status, and plans for future enhancements.

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