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    Fast Holographic Deconvolution: A New Technique for Precision Radio Interferometry

    189882_72953_71788_____0004-637X_759_1_17.pdf (1.236Mb)
    Access Status
    Open access
    Authors
    Sullivan, I.
    Morales, M.
    Hazelton, B.
    Arcus, Wayne
    Barnes, D.
    Bernardi, G.
    Briggs, F.
    Bowman, J.
    Bunton, J.
    Cappallo, R.
    Corey, B.
    Deshpande, A.
    DeSouza, L.
    Emrich, David
    Gaensler, B.
    Goeke, R.
    Greenhill, L.
    Herne, David
    Hewitt, J.
    Johnston-Hollitt, M.
    Kaplan, D.
    Kasper, J.
    Kincaid, B.
    Koenig, R.
    Kratzenberg, E.
    Lonsdale, C.
    Lynch, Mervyn
    McWhirter, S.
    Mitchell, D.
    Morgan, E.
    Oberoi, D.
    Ord, Stephen
    Pathikulangara, J.
    Prabu, T.
    Remillard, R.
    Rogers, A.
    Salah, J.
    Sault, R.
    Shankar, N.
    Srivani, K.
    Stevens, J.
    Subrahmanyan, R.
    Tingay, Steven
    Wayth, Randall
    Waterson, Mark
    Webster, R.
    Whitney, A.
    Date
    2012
    Type
    Journal Article
    
    Metadata
    Show full item record
    Citation
    Sullivan, I and Morales, M and Hazelton, B and Arcus, W and Barnes, D and Bernardi, G and Briggs, F and Bowman, J. et al. 2012. Fast Holographic Deconvolution: A New Technique for Precision Radio Interferometry. Astrophysical Journal 759: 17 (6 pp).
    Source Title
    The Astrophysical Journal
    DOI
    10.1088/0004-637X/759/1/17
    ISSN
    0004637X
    School
    Curtin Institute of Radio Astronomy (Physics)
    URI
    http://hdl.handle.net/20.500.11937/13706
    Collection
    • Curtin Research Publications
    Abstract

    We introduce the Fast Holographic Deconvolution method for analyzing interferometric radio data. Our new method is an extension of A-projection/software-holography/forward modeling analysis techniques and shares their precision deconvolution and wide-field polarimetry, while being significantly faster than current implementations that use full direction-dependent antenna gains. Using data from the MWA 32 antenna prototype, we demonstrate the effectiveness and precision of our new algorithm. Fast Holographic Deconvolution may be particularly important for upcoming 21 cm cosmology observations of the Epoch of Reionization and Dark Energy where foreground subtraction is intimately related to the precision of the data reduction.

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