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dc.contributor.authorMurphy, T.
dc.contributor.authorKaplan, D.
dc.contributor.authorBell, M.
dc.contributor.authorCallingham, J.
dc.contributor.authorCroft, S.
dc.contributor.authorJohnston, S.
dc.contributor.authorDobie, D.
dc.contributor.authorZic, A.
dc.contributor.authorHughes, J.
dc.contributor.authorLynch, C.
dc.contributor.authorHancock, P.
dc.contributor.authorHurley-Walker, Natasha
dc.contributor.authorLenc, E.
dc.contributor.authorDwarakanath, K.
dc.contributor.authorFor, B.
dc.contributor.authorGaensler, B.
dc.contributor.authorHindson, L.
dc.contributor.authorJohnston-Hollitt, M.
dc.contributor.authorKapinska, A.
dc.contributor.authorMcKinley, B.
dc.contributor.authorMorgan, J.
dc.contributor.authorOffringa, A.
dc.contributor.authorProcopio, P.
dc.contributor.authorStaveley-Smith, L.
dc.contributor.authorWayth, Randall
dc.contributor.authorWu, C.
dc.contributor.authorZheng, Q.
dc.identifier.citationMurphy, T. and Kaplan, D. and Bell, M. and Callingham, J. and Croft, S. and Johnston, S. and Dobie, D. et al. 2017. Low-Frequency Spectral Energy Distributions of Radio Pulsars Detected with the Murchison Widefield Array. Publications of the Astronomical Society of Australia. 34: Article ID e020.

We present low-frequency spectral energy distributions of 60 known radio pulsars observed with the Murchison Widefield Array telescope. We searched the GaLactic and Extragalactic All-sky Murchison Widefield Array survey images for 200-MHz continuum radio emission at the position of all pulsars in the Australia Telescope National Facility (ATNF) pulsar catalogue. For the 60 confirmed detections, we have measured flux densities in 20 × 8 MHz bands between 72 and 231 MHz. We compare our results to existing measurements and show that the Murchison Widefield Array flux densities are in good agreement.

dc.publisherCambridge University Press
dc.titleLow-Frequency Spectral Energy Distributions of Radio Pulsars Detected with the Murchison Widefield Array
dc.typeJournal Article
dcterms.source.titlePublications of the Astronomical Society of Australia

This article has been published in a revised form in Astronomical Society of Australia 10.1017/pasa.2017.13 This version is free to view and download for private research and study only. Not for re-distribution, re-sale or use in derivative works

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

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