A Bayesian method to mitigate the effects of unmodelled time-varying systematics for 21-cm cosmology experiments
Author:
Affiliation:
1. Astrophysics Group, Cavendish Laboratory , J. J. Thomson Avenue, Cambridge CB3 0HE , UK
2. Kavli Institute for Cosmology , Madingley Road, Cambridge CB3 0HA , UK
Abstract
Funder
Science and Technology Facilities Council
Kavli Foundation
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
https://academic.oup.com/mnras/advance-article-pdf/doi/10.1093/mnras/stad3725/53972831/stad3725.pdf
Reference55 articles.
1. A general Bayesian framework for foreground modelling and chromaticity correction for global 21 cm experiments
2. Possible interaction between baryons and dark-matter particles revealed by the first stars
3. Foregrounds for observations of the cosmological 21 cm line
4. maxsmooth: rapid maximally smooth function fitting with applications in Global 21-cm cosmology
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