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Verifying the low frequency pulsar polarimetry of the MWA

Published online by Cambridge University Press:  04 June 2018

Steven E. Tremblay
Affiliation:
International Centre for Radio Astronomy Research (ICRAR), Curtin University, Bentley, WA 6102, Australia email: steven.tremblay@curtin.edu.au ARC Centre of Excellence for All-sky Astrophysics (CAASTRO)
Mengyao Xue
Affiliation:
International Centre for Radio Astronomy Research (ICRAR), Curtin University, Bentley, WA 6102, Australia email: steven.tremblay@curtin.edu.au ARC Centre of Excellence for All-sky Astrophysics (CAASTRO)
N. D. Ramesh Bhat
Affiliation:
International Centre for Radio Astronomy Research (ICRAR), Curtin University, Bentley, WA 6102, Australia email: steven.tremblay@curtin.edu.au ARC Centre of Excellence for All-sky Astrophysics (CAASTRO)
Caterina Tiburzi
Affiliation:
Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, 53121 Bonn, Germany Universität Bielefeld, Fakultät für Physik, Universitätsstr. 25, D-33615 Bielefeld, Germany
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Abstract

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Studying 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.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2018 

References

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