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Galactic foreground science: Faraday Tomography at low frequencies

Published online by Cambridge University Press:  08 May 2018

Marijke Haverkorn Open the ORCID record for Marijke Haverkorn [Opens in a new window]
Marijke Haverkorn*
Affiliation:
Department of Astrophysics/IMAPP, Radboud University, Heyendaalseweg 135, 6525 AJ Nijmegen, The Netherlands email: m.haverkorn@astro.ru.nl
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Abstract

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This contribution describes how low-frequency radio-spectropolarimetric imaging as done for Epoch of Reionization detection is used to investigate the nearby Galactic interstellar medium. The method of Faraday Tomography allows disentangling of every line of sight into various components in Faraday depth, which is a proxy for density-weighted magnetic field. I discuss instrumental biases and side effects of this method, and early results it has yielded.

Keywords

ISM: magnetic fieldsISM: structuretechniques: polarimetricradio continuum: ISM
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 12 , Symposium S333: Peering towards Cosmic Dawn , October 2017 , pp. 129 - 137
Copyright
Copyright © International Astronomical Union 2018 

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