The radio environment of the 21 Centimeter Array: RFI detection and mitigation
Yan Huang, Xiang-Ping Wu, Qian Zheng, Jun-Hua Gu, Haiguang Xu

TL;DR
This paper presents effective RFI detection and mitigation techniques for the 21 Centimeter Array, crucial for low frequency radio observations targeting cosmic dawn and reionization, using statistical and innovative visibility correlation methods.
Contribution
It introduces a statistical RFI identification approach and the visibility correlation coefficient to improve RFI suppression in low frequency radio interferometry.
Findings
State-of-the-art techniques effectively mitigate RFI in 21CMA data.
Visibility correlation coefficient enhances suppression of time-varying RFI.
Mitigation methods enable more accurate cosmic signal detection.
Abstract
Detection and mitigation of radio frequency interference (RFI) is the first and also the key step for data processing in radio observations, especially for ongoing low frequency radio experiments towards the detection of the cosmic dawn and epoch of reionization (EoR). In this paper we demonstrate the technique and efficiency of RFI identification and mitigation for the 21 Centimeter Array (21CMA), a radio interferometer dedicated to the statistical measurement of EoR. For terrestrial, man-made RFI, we concentrate mainly on a statistical approach by identifying and then excising non-Gaussian signatures, in the sense that the extremely weak cosmic signal is actually buried under thermal and therefore Gaussian noise. We also introduce the so-called visibility correlation coefficient instead of conventional visibility, which allows a further suppression of rapidly time-varying RFI.…
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.
