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dc.contributor.authorProcopio, P.
dc.contributor.authorWayth, R. B.
dc.contributor.authorLine, J.
dc.contributor.authorTrott, C. M.
dc.contributor.authorIntema, Huib T.
dc.contributor.authorMitchell, D. A.
dc.contributor.authorPindor, B.
dc.contributor.authorRiding, J.
dc.contributor.authorTingay, S. J.
dc.contributor.authorBell, M. E.
dc.contributor.authorCallingham, J. R.
dc.contributor.authorDwarakanath, K. S.
dc.contributor.authorFor, Bi-Qing
dc.contributor.authorGaensler, B. M.
dc.contributor.authorHancock, P. J.
dc.contributor.authorHindson, L.
dc.contributor.authorHurley-Walker, N.
dc.contributor.authorJohnston-Hollitt, M.
dc.contributor.authorKapińnska, A. D.
dc.contributor.authorLenc, E.
dc.contributor.authorMcKinley, B.
dc.contributor.authorMorgan, J.
dc.contributor.authorOffringa, A.
dc.contributor.authorStaveley-Smith, L.
dc.contributor.authorWu, Chen
dc.contributor.authorZheng, Q.
dc.date.accessioned2017-08-16T16:32:38Z
dc.date.available2017-08-16T16:32:38Z
dc.date.issued2017-08-10
dc.identifier.citationProcopio , P , Wayth , R B , Line , J , Trott , C M , Intema , H T , Mitchell , D A , Pindor , B , Riding , J , Tingay , S J , Bell , M E , Callingham , J R , Dwarakanath , K S , For , B-Q , Gaensler , B M , Hancock , P J , Hindson , L , Hurley-Walker , N , Johnston-Hollitt , M , Kapińnska , A D , Lenc , E , McKinley , B , Morgan , J , Offringa , A , Staveley-Smith , L , Wu , C & Zheng , Q 2017 , ' A high resolution foreground model for the MWA EoR1 field : model and implications for EoR power spectrum analysis ' , Publications of the Astronomical Society of Australia , vol. 34 , E033 . https://doi.org/10.1017/pasa.2017.26
dc.identifier.issn1323-3580
dc.identifier.otherPURE: 12280308
dc.identifier.otherPURE UUID: 5d45a33e-ed75-4f7a-bdec-8dc335313f34
dc.identifier.otherArXiv: http://arxiv.org/abs/1707.02288v1
dc.identifier.otherScopus: 85093583078
dc.identifier.urihttp://hdl.handle.net/2299/19232
dc.descriptionThis article has been published in a revised form in Publications of the Astronomical Society of Australia https://doi.org/10.1017/pasa.2017.26 This version is free to view and download for private research and study only. Not for re-distribution, re-sale or use in derivative works. Under embargo. Embargo end date: 10 February 2018. © Astronomical Society of Australia 2017.
dc.description.abstractThe current generation of experiments aiming to detect the neutral hydrogen signal from the Epoch of Reionisation (EoR) is likely to be limited by systematic effects associated with removing foreground sources from target fields. In this paper we develop a model for the compact foreground sources in one of the target fields of the MWA's EoR key science experiment: the `EoR1' field. The model is based on both the MWA's GLEAM survey and GMRT 150 MHz data from the TGSS survey, the latter providing higher angular resolution and better astrometric accuracy for compact sources than is available from the MWA alone. The model contains 5049 sources, some of which have complicated morphology in MWA data, Fornax A being the most complex. The higher resolution data show that 13% of sources that appear point-like to the MWA have complicated morphology such as double and quad structure, with a typical separation of 33~arcsec. We derive an analytic expression for the error introduced into the EoR two-dimensional power spectrum due to peeling close double sources as single point sources and show that for the measured source properties, the error in the power spectrum is confined to high $k_\bot$ modes that do not affect the overall result for the large-scale cosmological signal of interest. The brightest ten mis-modelled sources in the field contribute 90% of the power bias in the data, suggesting that it is most critical to improve the models of the brightest sources. With this hybrid model we reprocess data from the EoR1 field and show a maximum of 8% improved calibration accuracy and a factor of two reduction in residual power in $k$-space from peeling these sources. Implications for future EoR experiments including the SKA are discussed in relation to the improvements obtained.en
dc.language.isoeng
dc.relation.ispartofPublications of the Astronomical Society of Australia
dc.rightsEmbargoed
dc.subjectastro-ph.IM
dc.titleA high resolution foreground model for the MWA EoR1 field : model and implications for EoR power spectrum analysisen
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.description.statusPeer reviewed
dc.date.embargoedUntil2018-02-10
dc.description.versiontypeFinal Accepted Version
dcterms.dateAccepted2017-08-10
rioxxterms.versionAM
rioxxterms.versionofrecordhttps://doi.org/10.1017/pasa.2017.26
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue
herts.rights.accesstypeEmbargoed


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