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    The EoR sensitivity of the Murchison Widefield Array

    193846_98659_MNRAS-2013-Beardsley-L5-9_1_.pdf (508.3Kb)
    Access Status
    Open access
    Authors
    Arcus, Wayne
    Emrich, David
    Herne, David
    Lynch, Mervyn
    Tingay, Steven
    Wayth, Randall
    Waterson, Mark
    Beardsley, A.
    Hazelton, B.
    Morales, M.
    Barnes, D.
    Bernardi, G.
    Bowman, J.
    Briggs, F.
    Bunton, J.
    Cappallo, R.
    Corey, B.
    Deshpande, A.
    deSouza, L.
    Gaensler, B.
    Goeke, R.
    Greenhill, L.
    Hewitt, J.
    Johnston-Hollitt, M.
    Kaplan, D.
    Kasper, J.
    Kincaid, B.
    Koenig, R.
    Kratzenberg, E.
    Lonsdale, C.
    McWhirter, S.
    Mitchell, D.
    Morgan, E.
    Oberoi, D.
    Ord, S.
    Pathikulangara, J.
    Prabu, T.
    Remillard, R.
    Rogers, A.
    Roshi, A.
    Salah, J.
    Sault, R.
    Udaya Shankar, N.
    Srivani, K.
    Stevens, J.
    Subrahmanyan, R.
    Webster, R.
    Whitney, A.
    Williams, A.
    Williams, C.
    Wyithe, J.
    Date
    2013
    Type
    Journal Article
    
    Metadata
    Show full item record
    Citation
    Beardsley, A.P. and Hazelton, B.J. and Morales, M.F. and Arcus, W. and Barnes, D. and Bernardi, G. and Bowman, J.D. et al. 2013. The EoR sensitivity of the Murchison Widefield Array. Monthly Notices of the Royal Astronomical Society: Letters. 429 (1): pp. L5-L9.
    Source Title
    Monthly Notices of the Royal Astronomical Society: Letters
    DOI
    10.1093/mnrasl/sls013
    ISSN
    1745-3925
    Remarks

    Copyright © 2012 The Authors. Published by Oxford University Press on behalf of Royal Astronomical Society. All rights reserved.

    URI
    http://hdl.handle.net/20.500.11937/4298
    Collection
    • Curtin Research Publications
    Abstract

    Using the final 128 antenna locations of the Murchison Widefield Array (MWA), we calculate its sensitivity to the epoch of reionization (EoR) power spectrum of redshifted 21 cm emission for a fiducial model and provide the tools to calculate the sensitivity for any model. Our calculation takes into account synthesis rotation, chromatic and asymmetrical baseline effects, and excludes modes that will be contaminated by foreground subtraction. For the fiducial model, the MWA will be capable of a 14s detection of the EoR signal with one full season of observation on two fields (900 and 700 h).

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