Foreground removal in HI 21 cm intensity mapping under frequency-dependent beam distortions
Athanasia Gkogkou, Victor Bonjean, Jean-Luc Starck, Marta Spinelli, Panagiotis Tsakalides

TL;DR
This paper evaluates the robustness of the SDecGMCA method for foreground removal in HI 21 cm intensity mapping, demonstrating its superior performance under realistic, frequency-dependent beam distortions compared to other techniques.
Contribution
It introduces and assesses the SDecGMCA method, extending DecGMCA to spherical data for effective foreground removal under complex beam conditions.
Findings
SDecGMCA remains robust with frequency-dependent beam distortions.
It suppresses spectral artifacts better than other methods.
Achieves less than 5% accuracy at intermediate scales.
Abstract
Neutral hydrogen (HI) intensity mapping with single-dish experiments is a powerful approach for probing cosmology in the post-reionization epoch. However, the presence of bright foregrounds over four orders of magnitude stronger than the HI signal makes its extraction highly challenging. While all methods perform well when assuming a Gaussian beam degraded to the worst resolution, most of them degrade significantly in the presence of a more realistic beam model. In this work, we investigate the performance of SDecGMCA. This method extends DecGMCA to spherical data, combining sparse component separation with beam deconvolution. Our goal is to evaluate this method in comparison with established foreground removal techniques, assessing its ability to recover the cosmological HI signal from single-dish intensity mapping observations under varying beam conditions. We use simulated HI signal…
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Taxonomy
TopicsRadio Astronomy Observations and Technology · Cosmology and Gravitation Theories · Galaxies: Formation, Evolution, Phenomena
