Global 21-cm signal extraction from foreground and instrumental effects I: Pattern recognition framework for separation using training sets
Keith Tauscher, David Rapetti, Jack O. Burns, Eric R. Switzer

TL;DR
This paper introduces a novel signal extraction method for global 21-cm cosmology experiments using SVD of training sets to effectively separate the cosmological signal from complex foregrounds and systematics, implemented in an open-source Python package.
Contribution
It presents a new SVD-based framework for separating the 21-cm signal from systematics, which does not require precise absolute knowledge of systematics, only their variability.
Findings
The method effectively isolates the 21-cm signal in simulated data.
Minimizing the Deviance Information Criterion yields unbiased signal estimates.
The approach is implemented in the publicly available 'pylinex' Python package.
Abstract
The sky-averaged (global) highly redshifted 21-cm spectrum from neutral hydrogen is expected to appear in the VHF range of MHz and its spectral shape and strength are determined by the heating properties of the first stars and black holes, by the nature and duration of reionization, and by the presence or absence of exotic physics. Measurements of the global signal would therefore provide us with a wealth of astrophysical and cosmological knowledge. However, the signal has not yet been detected because it must be seen through strong foregrounds weighted by a large beam, instrumental calibration errors, and ionospheric, ground and radio-frequency-interference effects, which we collectively refer to as "systematics". Here, we present a signal extraction method for global signal experiments which uses Singular Value Decomposition (SVD) of "training sets" to produce systematics…
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