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dc.contributor.authorOffringa, A. R.
dc.contributor.authorTrott, C. M.
dc.contributor.authorHurley-Walker, N.
dc.contributor.authorJohnston-Hollitt, M.
dc.contributor.authorMcKinley, B.
dc.contributor.authorBarry, N.
dc.contributor.authorBeardsley, A. P.
dc.contributor.authorBowman, J. D.
dc.contributor.authorBriggs, F.
dc.contributor.authorCarroll, P.
dc.contributor.authorGaensler, B. M.
dc.contributor.authorGreenhill, L. J.
dc.contributor.authorHazelton, B. J.
dc.contributor.authorJacobs, D. C.
dc.contributor.authorKim, H.-S.
dc.contributor.authorKittiwisit, P.
dc.contributor.authorLenc, E.
dc.contributor.authorLine, J.
dc.contributor.authorLoeb, A.
dc.contributor.authorMitchell, D. A.
dc.contributor.authorMorales, M. F.
dc.contributor.authorPaul, S.
dc.contributor.authorPindor, B.
dc.contributor.authorPober, J. C.
dc.contributor.authorProcopio, P.
dc.contributor.authorRiding, J.
dc.contributor.authorSethi, S. K.
dc.contributor.authorShankar, N. U.
dc.contributor.authorSubrahmanyan, R.
dc.contributor.authorSullivan, I. S.
dc.contributor.authorThyagarajan, N.
dc.contributor.authorTingay, S. J.
dc.contributor.authorWayth, R. B.
dc.contributor.authorWebster, R. L.
dc.contributor.authorWyithe, J. S. B.
dc.contributor.authorDillon, Joshua Shane
dc.contributor.authorEwall-Wice, Aaron Michael
dc.contributor.authorFeng, Lu
dc.contributor.authorHewitt, Jacqueline N
dc.contributor.authorNeben, Abraham Richard
dc.contributor.authorTegmark, Max Erik
dc.date.accessioned2017-04-19T17:50:16Z
dc.date.available2017-04-19T17:50:16Z
dc.date.issued2016-02
dc.date.submitted2016-02
dc.identifier.issn0035-8711
dc.identifier.issn1365-2966
dc.identifier.urihttp://hdl.handle.net/1721.1/108258
dc.description.abstractExperiments that pursue detection of signals from the Epoch of Reionization (EoR) are relying on spectral smoothness of source spectra at low frequencies. This article empirically explores the effect of foreground spectra on EoR experiments by measuring high-resolution full-polarization spectra for the 586 brightest unresolved sources in one of the Murchison Widefield Array (MWA) EoR fields using 45 h of observation. A novel peeling scheme is used to subtract 2500 sources from the visibilities with ionospheric and beam corrections, resulting in the deepest, confusion-limited MWA image so far. The resulting spectra are found to be affected by instrumental effects, which limit the constraints that can be set on source-intrinsic spectral structure. The sensitivity and power-spectrum of the spectra are analysed, and it is found that the spectra of residuals are dominated by point spread function sidelobes from nearby undeconvolved sources. We release a catalogue describing the spectral parameters for each measured source.en_US
dc.language.isoen_US
dc.publisherOxford University Pressen_US
dc.relation.isversionofhttp://dx.doi.org/10.1093/mnras/stw310en_US
dc.rightsCreative Commons Attribution-Noncommercial-Share Alikeen_US
dc.rights.urihttp://creativecommons.org/licenses/by-nc-sa/4.0/en_US
dc.sourcearXiven_US
dc.titleParametrizing Epoch of Reionization foregrounds: a deep survey of low-frequency point-source spectra with the Murchison Widefield Arrayen_US
dc.typeArticleen_US
dc.identifier.citationOffringa, A. R.; Trott, C. M.; Hurley-Walker, N.; Johnston-Hollitt, M.; McKinley, B.; Barry, N.; Beardsley, A. P. et al. “Parametrizing Epoch of Reionization Foregrounds: a Deep Survey of Low-Frequency Point-Source Spectra with the Murchison Widefield Array.” Monthly Notices of the Royal Astronomical Society 458, no. 1 (February 11, 2016): 1057–1070. © 2016 The Authorsen_US
dc.contributor.departmentMassachusetts Institute of Technology. Department of Physicsen_US
dc.contributor.departmentMIT Kavli Institute for Astrophysics and Space Researchen_US
dc.contributor.mitauthorDillon, Joshua Shane
dc.contributor.mitauthorEwall-Wice, Aaron Michael
dc.contributor.mitauthorFeng, Lu
dc.contributor.mitauthorHewitt, Jacqueline N
dc.contributor.mitauthorNeben, Abraham Richard
dc.contributor.mitauthorTegmark, Max Erik
dc.relation.journalMonthly Notices of the Royal Astronomical Societyen_US
dc.eprint.versionAuthor's final manuscripten_US
dc.type.urihttp://purl.org/eprint/type/JournalArticleen_US
eprint.statushttp://purl.org/eprint/status/PeerRevieweden_US
dspace.orderedauthorsOffringa, A. R.; Trott, C. M.; Hurley-Walker, N.; Johnston-Hollitt, M.; McKinley, B.; Barry, N.; Beardsley, A. P.; Bowman, J. D.; Briggs, F.; Carroll, P.; Dillon, J. S.; Ewall-Wice, A.; Feng, L.; Gaensler, B. M.; Greenhill, L. J.; Hazelton, B. J.; Hewitt, J. N.; Jacobs, D. C.; Kim, H.-S.; Kittiwisit, P.; Lenc, E.; Line, J.; Loeb, A.; Mitchell, D. A.; Morales, M. F.; Neben, A. R.; Paul, S.; Pindor, B.; Pober, J. C.; Procopio, P.; Riding, J.; Sethi, S. K.; Shankar, N. U.; Subrahmanyan, R.; Sullivan, I. S.; Tegmark, M.; Thyagarajan, N.; Tingay, S. J.; Wayth, R. B.; Webster, R. L.; Wyithe, J. S. B.en_US
dspace.embargo.termsNen_US
dc.identifier.orcidhttps://orcid.org/0000-0003-3336-9958
dc.identifier.orcidhttps://orcid.org/0000-0002-0086-7363
dc.identifier.orcidhttps://orcid.org/0000-0003-0422-2324
dc.identifier.orcidhttps://orcid.org/0000-0002-4117-570X
dc.identifier.orcidhttps://orcid.org/0000-0001-7776-7240
dc.identifier.orcidhttps://orcid.org/0000-0001-7670-7190
mit.licenseOPEN_ACCESS_POLICYen_US


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