Published in

Cambridge University Press (CUP), Proceedings of the International Astronomical Union, S337(13), p. 416-417

DOI: 10.1017/s174392131701033x

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Verifying the low frequency pulsar polarimetry of the MWA

Journal article published in 2017 by Steven E. Tremblay, Mengyao Xue ORCID, N. D. Ramesh Bhat, Caterina Tiburzi
This paper was not found in any repository, but could be made available legally by the author.
This paper was not found in any repository, but could be made available legally by the author.

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Data provided by SHERPA/RoMEO

Abstract

AbstractStudying the polarised properties of pulsars has a rich history giving unique geometric information about pulsars as well as testing the theories of pulsar emission physics. Performing such studies with the MWA has the attraction that the percentage of linear polarisation of many pulsars increases as the observing frequency decreases. Here we discuss the strategies being employed to verify the polarimetric response of the MWA’s high time resolution data.