Low frequency spectral energy distributions of radio pulsars detected with the Murchison widefield array

Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/6735

Title:	Low frequency spectral energy distributions of radio pulsars detected with the Murchison widefield array
Authors:	Murphy, Tara Kaplan, D.L. Dwarakanath, K.S. +25 Co-authors
Keywords:	Pulsars
Issue Date:	26-Apr-2017
Publisher:	Cambridge University Press for Astronomical Society of Australia
Citation:	Publications of the Astronomical Society of Australia, 2017, Vol.34, e020
Abstract:	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.
Description:	Restricted Access. An open-access version is available at arXiv.org (one of the alternative locations)
URI:	http://hdl.handle.net/2289/6735
ISSN:	1323-3580 1448-6083(online)
Alternative Location:	http://adsabs.harvard.edu/abs/2017PASA...34...20M https://arxiv.org/abs/1704.00027 http://dx.doi.org/10.1017/pasa.2017.13
Copyright:	2017 Astronomical Society of Australia
Appears in Collections:	Research Papers (A&A)

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