Galactic synchrotron emissivity measurements between 250° MWA
dc.contributor.author | Su, H. | |
dc.contributor.author | Hurley-Walker, N. | |
dc.contributor.author | Jackson, C. A. | |
dc.contributor.author | McClure-Griffiths, N. M. | |
dc.contributor.author | Tingay, S. J. | |
dc.contributor.author | Hindson, L. | |
dc.contributor.author | Hancock, P. | |
dc.contributor.author | Wayth, R. B. | |
dc.contributor.author | Gaensler, B. M. | |
dc.contributor.author | Staveley-Smith, L. | |
dc.contributor.author | Morgan, J. | |
dc.contributor.author | Johnston-Hollitt, M. | |
dc.contributor.author | Lenc, E. | |
dc.contributor.author | Bell, M. E. | |
dc.contributor.author | Callingham, J. R. | |
dc.contributor.author | Dwarkanath, K. S. | |
dc.contributor.author | For, B. Q. | |
dc.contributor.author | Kapińska, A. D. | |
dc.contributor.author | McKinley, B. | |
dc.contributor.author | Offringa, A. R. | |
dc.contributor.author | Procopio, P. | |
dc.contributor.author | Wu, C. | |
dc.contributor.author | Zheng, Q. | |
dc.date.accessioned | 2017-03-02T16:52:49Z | |
dc.date.available | 2017-03-02T16:52:49Z | |
dc.date.issued | 2017-03-01 | |
dc.identifier.citation | Su , 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.issn | 0035-8711 | |
dc.identifier.other | ArXiv: http://arxiv.org/abs/1611.05446v1 | |
dc.identifier.uri | http://hdl.handle.net/2299/17665 | |
dc.description | This 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.abstract | Synchrotron 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^\circ | en |
dc.format.extent | 4681751 | |
dc.language.iso | eng | |
dc.relation.ispartof | Monthly Notices of the Royal Astronomical Society | |
dc.subject | astro-ph.GA | |
dc.title | Galactic synchrotron emissivity measurements between 250° MWA | en |
dc.contributor.institution | School of Physics, Astronomy and Mathematics | |
dc.description.status | Peer reviewed | |
dc.identifier.url | https://academic.oup.com/mnras/article-lookup/doi/10.1093/mnras/stw2959 | |
rioxxterms.versionofrecord | 10.1093/mnras/stw2959 | |
rioxxterms.type | Journal Article/Review | |
herts.preservation.rarelyaccessed | true |