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dc.contributor.authorJacobs, D.
dc.contributor.authorHazelton, B.
dc.contributor.authorTrott, C.
dc.contributor.authorDillon, J.
dc.contributor.authorPindor, B.
dc.contributor.authorSullivan, I.
dc.contributor.authorPober, J.
dc.contributor.authorBarry, N.
dc.contributor.authorBeardsley, A.
dc.contributor.authorBernardi, G.
dc.contributor.authorBowman, J.
dc.contributor.authorBriggs, F.
dc.contributor.authorCappallo, R.
dc.contributor.authorCarroll, P.
dc.contributor.authorCorey, B.
dc.contributor.authorOliveira-Costa, A.
dc.contributor.authorEmrich, D.
dc.contributor.authorEwall-Wice, A.
dc.contributor.authorFeng, L.
dc.contributor.authorGaensler, B.
dc.contributor.authorGoeke, R.
dc.contributor.authorGreenhill, L.
dc.contributor.authorHewitt, J.
dc.contributor.authorHurley-Walker, N.
dc.contributor.authorJohnston-Hollitt, M.
dc.contributor.authorKaplan, D.
dc.contributor.authorKasper, J.
dc.contributor.authorKim, H.
dc.contributor.authorKratzenberg, E.
dc.contributor.authorLenc, E.
dc.contributor.authorLine, J.
dc.contributor.authorLoeb, A.
dc.contributor.authorLonsdale, C.
dc.contributor.authorLynch, M.
dc.contributor.authorMcKinley, B.
dc.contributor.authorMcWhirter, S.
dc.contributor.authorMitchell, D.
dc.contributor.authorMorales, M.
dc.contributor.authorMorgan, E.
dc.contributor.authorNeben, A.
dc.contributor.authorThyagarajan, N.
dc.contributor.authorOberoi, D.
dc.contributor.authorOffringa, A.
dc.contributor.authorOrd, S.
dc.contributor.authorPaul, S.
dc.contributor.authorPrabu, T.
dc.contributor.authorProcopio, P.
dc.contributor.authorRiding, J.
dc.contributor.authorRogers, A.
dc.contributor.authorRoshi, A.
dc.contributor.authorShankar, N.
dc.contributor.authorSethi, S.
dc.contributor.authorSrivani, K.
dc.contributor.authorSubrahmanyan, R.
dc.contributor.authorTegmark, M.
dc.contributor.authorTingay, Steven
dc.contributor.authorWaterson, M.
dc.contributor.authorWayth, Randall
dc.contributor.authorWebster, R.
dc.contributor.authorWhitney, A.
dc.contributor.authorWilliams, A.
dc.contributor.authorWilliams, C.
dc.contributor.authorWu, C.
dc.contributor.authorWyithe, J.
dc.date.accessioned2017-01-30T12:14:43Z
dc.date.available2017-01-30T12:14:43Z
dc.date.created2016-07-31T19:31:03Z
dc.date.issued2016
dc.identifier.citationJacobs, D. and Hazelton, B. and Trott, C. and Dillon, J. and Pindor, B. and Sullivan, I. and Pober, J. et al. 2016. The murchison widefield array 21 cm power spectrum analysis methodology. Astrophysical Journal. 825 (2): Article ID 114.
dc.identifier.urihttp://hdl.handle.net/20.500.11937/19602
dc.identifier.doi10.3847/0004-637X/825/2/114
dc.description.abstract

We present the 21 cm power spectrum analysis approach of the Murchison Widefield Array Epoch of Reionization project. In this paper, we compare the outputs of multiple pipelines for the purpose of validating statistical limits cosmological hydrogen at redshifts between 6 and 12. Multiple independent data calibration and reduction pipelines are used to make power spectrum limits on a fiducial night of data. Comparing the outputs of imaging and power spectrum stages highlights differences in calibration, foreground subtraction, and power spectrum calculation. The power spectra found using these different methods span a space defined by the various tradeoffs between speed, accuracy, and systematic control. Lessons learned from comparing the pipelines range from the algorithmic to the prosaically mundane; all demonstrate the many pitfalls of neglecting reproducibility. We briefly discuss the way these different methods attempt to handle the question of evaluating a significant detection in the presence of foregrounds.

dc.publisherInstitute of Physics Publishing
dc.titleThe murchison widefield array 21 cm power spectrum analysis methodology
dc.typeJournal Article
dcterms.source.volume825
dcterms.source.number2
dcterms.source.issn0004-637X
dcterms.source.titleAstrophysical Journal
curtin.departmentCurtin Institute of Radio Astronomy (Physics)
curtin.accessStatusOpen access


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