Abstract
Abstract
We demonstrate the effectiveness of a Bayesian evidence -based analysis for diagnosing and disentangling the sky-averaged 21-cm signal from instrumental systematic effects. As a case study, we consider a simulated REACH pipeline with an injected systematic. We demonstrate that very poor performance or erroneous signal recovery is achieved if the systematic remains unmodelled. These effects include sky-averaged 21-cm posterior estimates resembling a very deep or wide signal. However, when including parameterised models of the systematic, the signal recovery is dramatically improved in performance. Most importantly, a Bayesian evidence-based model comparison is capable of determining whether or not such a systematic model is needed as the true underlying generative model of an experimental dataset is in principle unknown. We, therefore, advocate a pipeline capable of testing a variety of potential systematic errors with the Bayesian evidence acting as the mechanism for detecting their presence.
Publisher
Cambridge University Press (CUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Reference54 articles.
1. Handley, W. J. , Hobson, M. P. , & Lasenby, A. N. 2015b, MNRAS, 453, 4385
2. Elsherbeni, A. Z. a. 2014, Antenna Analysis and Design Using FEKO Electromagnetic Simulation Software (Edison, NJ: SciTech Publishing), an imprint of the IET, [2014] ©2014, https://search.library.wisc.edu/catalog/9910210974002121
3. Kraus, J. D. , Tiuri, M. , Räisänen, A. V. , & Carr, T. D. 1986, Radio Astronomy (Cygnus-Quasar Books)
4. Handley, W. J. , Hobson, M. P. , & Lasenby, A. N. 2015a, MNRASL, 450, L61
5. What does the first highly redshifted 21-cm detection tell us about early galaxies?
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