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dc.contributor.authorSu, H.
dc.contributor.authorHurley-Walker, N.
dc.contributor.authorJackson, C. A.
dc.contributor.authorMcClure-Griffiths, N. M.
dc.contributor.authorTingay, S. J.
dc.contributor.authorHindson, L.
dc.contributor.authorHancock, P.
dc.contributor.authorWayth, R. B.
dc.contributor.authorGaensler, B. M.
dc.contributor.authorStaveley-Smith, L.
dc.contributor.authorMorgan, J.
dc.contributor.authorJohnston-Hollitt, M.
dc.contributor.authorLenc, E.
dc.contributor.authorBell, M. E.
dc.contributor.authorCallingham, J. R.
dc.contributor.authorDwarkanath, K. S.
dc.contributor.authorFor, B. Q.
dc.contributor.authorKapińska, A. D.
dc.contributor.authorMcKinley, B.
dc.contributor.authorOffringa, A. R.
dc.contributor.authorProcopio, P.
dc.contributor.authorWu, C.
dc.contributor.authorZheng, Q.
dc.date.accessioned2017-03-02T16:52:49Z
dc.date.available2017-03-02T16:52:49Z
dc.date.issued2017-03-01
dc.identifier.citationSu , H , Hurley-Walker , N , Jackson , C A , McClure-Griffiths , N M , Tingay , S J , Hindson , L , Hancock , P , Wayth , R B , Gaensler , B M , Staveley-Smith , L , Morgan , J , Johnston-Hollitt , M , Lenc , E , Bell , M E , Callingham , J R , Dwarkanath , K S , For , B Q , Kapińska , A D , McKinley , B , Offringa , A R , Procopio , P , Wu , C & Zheng , Q 2017 , ' Galactic synchrotron emissivity measurements between 250° MWA ' , Monthly Notices of the Royal Astronomical Society , vol. 465 , no. 3 , pp. 3163-3174 . https://doi.org/10.1093/mnras/stw2959
dc.identifier.issn0035-8711
dc.identifier.otherArXiv: http://arxiv.org/abs/1611.05446v1
dc.identifier.urihttp://hdl.handle.net/2299/17665
dc.descriptionThis article has been accepted for publication in Monthly Notices of the Royal Astronomical Society following peer review. The version of record, H. Su et al, 'Galactic synchrotron emissivity measurements between 250◦ < l < 355◦ from the GLEAM survey with the MWA', MNRAS, 465(3): 3163-3174, first published online 17 November 2016, is available via doi: 10.1093/mnras/stw2959. © : 2016 The Authors. Published by Oxford University Press on behalf of the Royal Astronomical Society.
dc.description.abstractSynchrotron emission pervades the Galactic plane at low radio frequencies, originating from cosmic ray electrons interacting with the Galactic magnetic field. Using a low-frequency radio telescope, the Murchison Widefield Array (MWA), we measure the free-free absorption of this Galactic synchrotron emission by intervening HII regions along the line of sight. These absorption measurements allow us to calculate the Galactic cosmic-ray electron emissivity behind and in front of 47 detected HII regions in the region $250^\circen
dc.format.extent4681751
dc.language.isoeng
dc.relation.ispartofMonthly Notices of the Royal Astronomical Society
dc.subjectastro-ph.GA
dc.titleGalactic synchrotron emissivity measurements between 250° MWAen
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.description.statusPeer reviewed
dc.identifier.urlhttps://academic.oup.com/mnras/article-lookup/doi/10.1093/mnras/stw2959
rioxxterms.versionofrecord10.1093/mnras/stw2959
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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