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    First season MWA EoR power spectrum results at redshift 7

    247548_247548.pdf (14.93Mb)
    Access Status
    Open access
    Authors
    Beardsley, A.
    Hazelton, B.
    Sullivan, I.
    Carroll, P.
    Barry, N.
    Rahimi, M.
    Pindor, B.
    Trott, Cathryn
    Line, J.
    Jacobs, D.
    Morales, M.
    Pober, J.
    Bernardi, G.
    Bowman, J.
    Busch, M.
    Briggs, F.
    Cappallo, R.
    Corey, B.
    Oliveira-Costa, A.
    Dillon, J.
    Emrich, David
    Ewall-Wice, A.
    Feng, L.
    Gaensler, B.
    Goeke, R.
    Greenhill, L.
    Hewitt, J.
    Hurley-Walker, Natasha
    Johnston-Hollitt, M.
    Kaplan, D.
    Kasper, J.
    Kim, H.
    Kratzenberg, E.
    Lenc, E.
    Loeb, A.
    Lonsdale, C.
    Lynch, Mervyn
    McKinley, B.
    McWhirter, S.
    Mitchell, D.
    Morgan, E.
    Neben, A.
    Thyagarajan, N.
    Oberoi, D.
    Offringa, A.
    Ord, S.
    Paul, S.
    Prabu, T.
    Procopio, P.
    Riding, J.
    Rogers, A.
    Roshi, A.
    Shankar, N.
    Sethi, S.
    Srivani, K.
    Subrahmanyan, R.
    Tegmark, M.
    Tingay, Steven
    Waterson, M.
    Wayth, Randall
    Webster, R.
    Whitney, A.
    Williams, Andrew
    Williams, C.
    Wu, C.
    Wyithe, J.
    Date
    2016
    Type
    Journal Article
    
    Metadata
    Show full item record
    Citation
    Beardsley, A. and Hazelton, B. and Sullivan, I. and Carroll, P. and Barry, N. and Rahimi, M. and Pindor, B. et al. 2016. First season MWA EOR power spectrum results at redshift 7. Astrophysical Journal. 833 (1): Article 102.
    Source Title
    Astrophysical Journal
    DOI
    10.3847/1538-4357/833/1/102
    ISSN
    0004-637X
    School
    Department of Electrical and Computer Engineering
    Remarks

    This is an author-created, un-copy edited version of an article accepted for publication in Astrophysical Journal. The publisher is not responsible for any errors or omissions in this version of the manuscript or any version derived from it. The Version of Record is available online at http://doi.org/10.3847/1538-4357/833/1/102

    URI
    http://hdl.handle.net/20.500.11937/21766
    Collection
    • Curtin Research Publications
    Abstract

    The Murchison Widefield Array (MWA) has collected hundreds of hours of Epoch of Reionization (EoR) data and now faces the challenge of overcoming foreground and systematic contamination to reduce the data to a cosmological measurement. We introduce several novel analysis techniques, such as cable reflection calibration, hyper-resolution gridding kernels, diffuse foreground model subtraction, and quality control methods. Each change to the analysis pipeline is tested against a two-dimensional power spectrum figure of merit to demonstrate improvement. We incorporate the new techniques into a deep integration of 32 hours of MWA data. This data set is used to place a systematic-limited upper limit on the cosmological power spectrum of ∆2 ≤ 2.7×104 mK2 at k =0.27 h Mpc-1 and z = 7.1, consistent with other published limits, and a modest improvement (factor of 1.4) over previous MWA results. From this deep analysis, we have identified a list of improvements to be made to our EoR data analysis strategies. These improvements will be implemented in the future and detailed in upcoming publications.

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