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Foreground Mitigation in the Epoch of Reionization

Published online by Cambridge University Press:  08 May 2018

Emma Chapman Open the ORCID record for Emma Chapman [Opens in a new window]
Emma Chapman*
Affiliation:
Astrophysics Group, Imperial College London, Blackett Laboratory, Prince Consort Road, London, SW7 2AZ, United Kingdom email: [email protected]
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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.

Keywords

methods: data analysismethods: statisticaltelescopesradio continuum: generalcosmology: observations(cosmology:) early universe
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 12 , Symposium S333: Peering towards Cosmic Dawn , October 2017 , pp. 261 - 268
Copyright
Copyright © International Astronomical Union 2018 

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