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Foreground Mitigation in the Epoch of Reionization

Published online by Cambridge University Press:  08 May 2018

Emma Chapman*
Affiliation:
Astrophysics Group, Imperial College London, Blackett Laboratory, Prince Consort Road, London, SW7 2AZ, United Kingdom email: e.chapman@imperial.ac.uk
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Abstract

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The EoR foregrounds can be up to three magnitudes greater than the cosmological signal we wish to detect. Multiple methods have been developed in order to extract the cosmological signal, falling roughly into three categories: foreground removal, foreground suppression and foreground avoidance. These main approaches are briefly discussed in this review and consideration taken to the future application of these methods as a multi-layered approach.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2018 

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