21cm Signal Recovery via the Robust Principle Component Analysis
Shifan Zuo, Xuelei Chen, Reza Ansari, Youjun Lu

TL;DR
This paper introduces a novel foreground subtraction method for 21cm cosmology signals using Robust Principal Component Analysis, leveraging both the low-rank and sparse properties to improve signal recovery.
Contribution
The paper presents the first application of sparsity of the 21cm signal's frequency covariance in RPCA for foreground removal, enhancing separation without signal loss.
Findings
Effective separation of foregrounds and 21cm signal demonstrated
Method applicable to both small patches and large sky areas
Robust to sky map defects and complex conditions
Abstract
The redshifted 21~cm signal from neutral hydrogen (HI) is potentially a very powerful probe for cosmology, but a difficulty in its observation is that it is much weaker than foreground radiation from the Milky Way as well as extragalactic radio sources. The foreground radiation at different frequencies are however coherent along one line of sight, and various methods of foreground subtraction based on this property have been proposed. In this paper, we present a new method based on the Robust Principal Component Analysis (RPCA) to subtract foreground and extract 21~cm signal, which explicitly uses both the low-rank property of the frequency covariance matrix (i.e. frequency coherence) of the foreground and the sparsity of the frequency covariance matrix of the 21~cm signal. The low-rank property of the foregrounds frequency covariance has been exploited in many previous works on…
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