摘要: 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.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
remove the foreground residual after the conservative PCA subtraction or
compensate for the signal loss caused by the aggressive PCA preprocessing.
Finally, we test the robustness of the U-Net foreground subtraction technique
and show that it is still reliable in the case of existing constraint error on
HI fluctuation amplitude.