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Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/6735
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dc.contributor.authorMurphy, Tara-
dc.contributor.authorKaplan, D.L.-
dc.contributor.authorDwarakanath, K.S.-
dc.contributor.author+25 Co-authors-
dc.date.accessioned2017-09-21T07:42:19Z-
dc.date.available2017-09-21T07:42:19Z-
dc.date.issued2017-04-26-
dc.identifier.citationPublications of the Astronomical Society of Australia, 2017, Vol.34, e020en_US
dc.identifier.issn1323-3580-
dc.identifier.issn1448-6083(online)-
dc.identifier.urihttp://hdl.handle.net/2289/6735-
dc.descriptionRestricted Access. An open-access version is available at arXiv.org (one of the alternative locations)en_US
dc.description.abstractWe 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.en_US
dc.language.isoenen_US
dc.publisherCambridge University Press for Astronomical Society of Australiaen_US
dc.relation.urihttp://adsabs.harvard.edu/abs/2017PASA...34...20Men_US
dc.relation.urihttps://arxiv.org/abs/1704.00027en_US
dc.relation.urihttp://dx.doi.org/10.1017/pasa.2017.13en_US
dc.rights2017 Astronomical Society of Australiaen_US
dc.subjectPulsarsen_US
dc.titleLow frequency spectral energy distributions of radio pulsars detected with the Murchison widefield arrayen_US
dc.typeArticleen_US
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