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    Wide-field broad-band radio imaging with phased array feeds: A pilot multi-epoch continuum survey with ASKAP-BETA

    240189_240189.pdf (7.177Mb)
    Access Status
    Open access
    Authors
    Heywood, I.
    Bannister, K.
    Marvil, J.
    Allison, J.
    Ball, L.
    Bell, M.
    Bock, D.
    Brothers, M.
    Bunton, J.
    Chippendale, A.
    Cooray, F.
    Cornwell, T.
    De Boer, D.
    Edwards, P.
    Gough, R.
    Gupta, N.
    Harvey-Smith, L.
    Hay, S.
    Hotan, A.
    Indermuehle, B.
    Jacka, C.
    Jackson, Carole
    Johnston, S.
    Kimball, A.
    Koribalski, B.
    Lenc, E.
    Macleod, A.
    McClure-Griffiths, N.
    McConnell, D.
    Mirtschin, P.
    Murphy, T.
    Neuhold, S.
    Norris, R.
    Pearce, S.
    Popping, A.
    Qiao, R.
    Reynolds, J.
    Sadler, E.
    Sault, R.
    Schinckel, A.
    Serra, P.
    Shimwell, T.
    Stevens, J.
    Tuthill, J.
    Tzioumis, A.
    Voronkov, M.
    Westmeier, T.
    Whiting, M.
    Date
    2016
    Type
    Journal Article
    
    Metadata
    Show full item record
    Citation
    Heywood, I. and Bannister, K. and Marvil, J. and Allison, J. and Ball, L. and Bell, M. and Bock, D. et al. 2016. Wide-field broad-band radio imaging with phased array feeds: A pilot multi-epoch continuum survey with ASKAP-BETA. Monthly Notices of the Royal Astronomical Society. 457 (4): pp. 4160-4178.
    Source Title
    Monthly Notices of the Royal Astronomical Society
    DOI
    10.1093/mnras/stw186
    ISSN
    0035-8711
    School
    Curtin Institute of Radio Astronomy (Physics)
    Remarks

    This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society ©: 2016 The Authors. Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.

    URI
    http://hdl.handle.net/20.500.11937/23267
    Collection
    • Curtin Research Publications
    Abstract

    The Boolardy Engineering TestArray is a 6×12mdish interferometer and the prototype of the Australian Square Kilometre Array Pathfinder (ASKAP), equipped with the first generation of ASKAP's phased array feed (PAF) receivers. These facilitate rapid wide-area imaging via the deployment of simultaneous multiple beams within an ~30 deg2 field of view. By cycling the array through 12 interleaved pointing positions and using nine digitally formed beams, we effectively mimic a traditional 1 h × 108 pointing survey, covering ~150 deg2 over 711-1015 MHz in 12 h of observing time. Three such observations were executed over the course of a week. We verify the full bandwidth continuum imaging performance and stability of the system via self-consistency checks and comparisons to existing radio data. The combined three epoch image has arcminute resolution and a 1s thermal noise level of 375 µJy beam-1, although the effective noise is a factor of ~3 higher due to residual sidelobe confusion. From this we derive a catalogue of 3722 discrete radio components, using the 35 per cent fractional bandwidth to measure in-band spectral indices for 1037 of them. A search for transient events reveals one significantly variable source within the survey area. The survey covers approximately two-thirds of the Spitzer South Pole Telescope Deep Field. This pilot project demonstrates the viability and potential of using PAFs to rapidly and accurately survey the sky at radio wavelengths.

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