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dc.contributor.authorMcKinley, B.
dc.contributor.authorBernardi, G.
dc.contributor.authorTrott, Cathryn
dc.contributor.authorLine, J.
dc.contributor.authorWayth, Randall
dc.contributor.authorOffringa, A.
dc.contributor.authorPindor, B.
dc.contributor.authorJordan, Christopher
dc.contributor.authorSokolowski, Marcin
dc.contributor.authorTingay, Steven
dc.contributor.authorLenc, E.
dc.contributor.authorHurley-Walker, Natasha
dc.contributor.authorBowman, J.
dc.contributor.authorBriggs, F.
dc.contributor.authorWebster, R.
dc.date.accessioned2019-02-19T04:15:42Z
dc.date.available2019-02-19T04:15:42Z
dc.date.created2019-02-19T03:58:21Z
dc.date.issued2018
dc.identifier.citationMcKinley, B. and Bernardi, G. and Trott, C. and Line, J. and Wayth, R. and Offringa, A. and Pindor, B. et al. 2018. Measuring the global 21-cm signal with the MWA-I: Improved measurements of the Galactic synchrotron background using lunar occultation. Monthly Notices of the Royal Astronomical Society. 481 (4): pp. 5034-5045.
dc.identifier.urihttp://hdl.handle.net/20.500.11937/74070
dc.identifier.doi10.1093/MNRAS/STY2437
dc.description.abstract

We present early results from a project to measure the sky-averaged (global), redshifted 21 cm signal from the Epoch of Reionization (EoR), using the Murchison Widefield Array (MWA) telescope. Because interferometers are not sensitive to a spatially invariant global average, they cannot be used to detect this signal using standard techniques.However, lunar occultation of the radio sky imprints a spatial structure on the global signal, allowing us to measure the average brightness temperature of the patch of sky immediately surrounding the Moon. In this paper, we present one night of Moon observations with the MWA between 72-230 MHz and verify our techniques to extract the background sky temperature from measurements of the Moon's flux density. We improve upon previous work using the lunar occultation technique by using a more sophisticated model for reflected 'earthshine' and by employing image differencing to remove imaging artefacts. We leave the Moon's (constant) radio brightness temperature as a free parameter in our fit to the data and as a result, measure Tmoon = 180 ± 12 K and a Galactic synchrotron spectral index of -2.64 ± 0.14, at the position of the Moon. Finally, we evaluate the prospects of the lunar occultation technique for a global EoR detection and map out a way forward for future work with the MWA.

dc.publisherOxford University Press
dc.titleMeasuring the global 21-cm signal with the MWA-I: Improved measurements of the Galactic synchrotron background using lunar occultation
dc.typeJournal Article
dcterms.source.volume481
dcterms.source.number4
dcterms.source.startPage5034
dcterms.source.endPage5045
dcterms.source.issn0035-8711
dcterms.source.titleMonthly Notices of the Royal Astronomical Society
curtin.note

This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society ©: 2018 The Authors. Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.

curtin.departmentCurtin Institute of Radio Astronomy (Physics)
curtin.accessStatusOpen access


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