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Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/5658
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dc.contributor.authorBeardsley, A. P.-
dc.contributor.authorHazelton, B.J.-
dc.contributor.authorMorales, M.F.-
dc.contributor.authorDeshpande, A.A.-
dc.contributor.authorPrabu, T.-
dc.contributor.authorRoshi, Anish D.-
dc.contributor.authorUdaya Shankar, N.-
dc.contributor.authorSrivani, K.S.-
dc.contributor.authorSubrahmanyan, Ravi-
dc.contributor.author+30 Co-authors-
dc.date.accessioned2013-06-26T05:58:44Z-
dc.date.available2013-06-26T05:58:44Z-
dc.date.issued2013-02-01-
dc.identifier.citationMonthly Notices of the Royal Astronomical Society Letters , 2013, Vol. 429, L5-L9en
dc.identifier.issn1745-3933 (online)-
dc.identifier.urihttp://hdl.handle.net/2289/5658-
dc.descriptionRestricted Access. An open-access version is available at arXiv.org (one of the alternative locations)en
dc.description.abstractUsing 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 14σ detection of the EoR signal with one full season of observation on two fields (900 and 700 h)en
dc.language.isoenen
dc.publisherOxford University Press for the Royal Astronomical Societyen
dc.relation.urihttp://adsabs.harvard.edu/abs/2013MNRAS.429L...5Ben
dc.relation.urihttp://arxiv.org/abs/1204.3111en
dc.relation.urihttp://dx.doi.org/10.1093/mnrasl/sls013en
dc.rights2013 The authors & the Royal Astronomical Society.en
dc.subjectinstrumentation: interferometersen
dc.subjectcosmology: miscellaneousen
dc.titleThe EoR sensitivity of the Murchison widefield arrayen
dc.typeArticleen
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