Eliminating polarization leakage effect for neutral hydrogen intensity mapping with deep learning
Li-Yang Gao, Yichao Li, Shulei Ni, Xin Zhang

TL;DR
This paper introduces a deep learning approach using U-Net to effectively remove polarization leakage effects in neutral hydrogen intensity mapping, improving foreground subtraction and signal recovery for large-scale structure studies.
Contribution
The study demonstrates that a U-Net deep learning model can enhance foreground removal in HI intensity mapping by addressing polarization leakage, outperforming traditional PCA methods.
Findings
U-Net effectively reduces polarization leakage residuals.
U-Net compensates for signal loss from PCA preprocessing.
Method remains robust under constraint errors on HI fluctuations.
Abstract
The neutral hydrogen (HI) intensity mapping (IM) survey is regarded as a promising approach for cosmic large-scale structure (LSS) studies. A major issue for the HI IM survey is to remove the bright foreground contamination. A key to successfully remove the bright foreground is to well control or eliminate the instrumental effects. In this work, we consider the instrumental effect of polarization leakage and use the U-Net approach, a deep learning-based foreground removal technique, to eliminate the polarization leakage effect. The thermal noise is assumed to be a subdominant factor compared with the polarization leakage for future HI IM surveys and ignored in this analysis. In this method, the principal component analysis (PCA) foreground subtraction is used as a preprocessing step for the U-Net foreground subtraction. Our results show that the additional U-Net processing could either…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsStellar, planetary, and galactic studies · Astronomical Observations and Instrumentation · Gamma-ray bursts and supernovae
