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dc.contributor.authorHindson, L.
dc.contributor.authorJohnston-Hollitt, M.
dc.contributor.authorHurley-Walker, N.
dc.contributor.authorMorgan, J.
dc.contributor.authorBuckley, K.
dc.contributor.authorCarretti, E.
dc.contributor.authorDwarakanath, K.
dc.contributor.authorBell, M.
dc.contributor.authorBernardi, G.
dc.contributor.authorBhat, R.
dc.contributor.authorBriggs, F.
dc.contributor.authorDeshpande, A.
dc.contributor.authorEwall-Wice, A.
dc.contributor.authorFeng, L.
dc.contributor.authorHazelton, B.
dc.contributor.authorJacobs, D.
dc.contributor.authorKaplan, D.
dc.contributor.authorKudryavtseva, N.
dc.contributor.authorLenc, E.
dc.contributor.authorMcKinley, B.
dc.contributor.authorMitchell, D.
dc.contributor.authorPindor, B.
dc.contributor.authorProcopio, P.
dc.contributor.authorOberoi, D.
dc.contributor.authorOffringa, A.
dc.contributor.authorOrd, S.
dc.contributor.authorRiding, J.
dc.contributor.authorBowman, J.
dc.contributor.authorCappallo, R.
dc.contributor.authorCorey, B.
dc.contributor.authorEmrich, D.
dc.contributor.authorGaensler, B.
dc.contributor.authorGoeke, R.
dc.contributor.authorGreenhill, L.
dc.contributor.authorKasper, J.
dc.contributor.authorKratzenberg, E.
dc.contributor.authorLonsdale, C.
dc.contributor.authorLynch, Mervyn
dc.contributor.authorMcWhirter, R.
dc.contributor.authorMorales, M.
dc.contributor.authorMorgan, E.
dc.contributor.authorPrabu, T.
dc.contributor.authorRogers, A.
dc.contributor.authorRoshi, A.
dc.contributor.authorShankar, U.
dc.contributor.authorSrivani, K.
dc.contributor.authorSubrahmanyan, R.
dc.contributor.authorTingay, Steven
dc.contributor.authorWaterson, M.
dc.contributor.authorWebster, R.
dc.contributor.authorWhitney, A.
dc.contributor.authorWilliams, A.
dc.contributor.authorWilliams, C.
dc.date.accessioned2017-01-30T14:25:48Z
dc.date.available2017-01-30T14:25:48Z
dc.date.created2015-10-29T04:09:19Z
dc.date.issued2014
dc.identifier.citationHindson, L. and Johnston-Hollitt, M. and Hurley-Walker, N. and Morgan, J. and Buckley, K. and Carretti, E. and Dwarakanath, K. et al. 2014. First look Murchison Widefield Array observations of Abell 3667, in Proceedings of the XXXIth URSI General Assembly and Scientific Symposium (URSI GASS), Aug 16-23 2014. Bejing: Institute of Electrical and Electronics Engineers Inc.
dc.identifier.urihttp://hdl.handle.net/20.500.11937/38756
dc.identifier.doi10.1109/URSIGASS.2014.6930053
dc.description.abstract

The Murchison Widefield Array (MWA) is a new low frequency interferometric radio telescope, operating in the remote Murchison Radio Observatory in Western Australia. In this paper we present the first MWA observations of the well known radio relics in Abell 3667 (A3667) between 120 and 226 MHz. We clearly detect the radio relics in A3667 and present flux estimates and spectral indices for these features. The average spectral index of the north-west (NW) and south-east (SE) relics is -0.9 ± 0.1 between 120 and 1400 MHz. We are able to resolve spatial variation in the spectral index of the NW relic from -1.7 to -0.4, which is consistent with results found at higher frequencies.

dc.publisherInstitute of Electrical and Electronics Engineers Inc.
dc.titleFirst look Murchison Widefield Array observations of Abell 3667
dc.typeConference Paper
dcterms.source.title2014 31th URSI General Assembly and Scientific Symposium, URSI GASS 2014
dcterms.source.series2014 31th URSI General Assembly and Scientific Symposium, URSI GASS 2014
dcterms.source.isbn9781467352253
curtin.departmentDepartment of Physics and Astronomy
curtin.accessStatusFulltext not available


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