Radio frequency interference identification using eigenvalue decomposition for multi-beam observations

Juntao Bai, Shi Dai, Na Wang, Stefan Osłowski, Shuangqiang Wang, George Hobbs, Jianping Yuan, Wenming Yan, Qijun Zhi, Lunhua Shang, Xin Xu, Shijun Dang, De Zhao

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Abstract

With the installation of next-generation phased array feed (PAF) receivers on radio telescopes, there is an urgent need to develop effective and computationally efficient radio frequency interference (RFI) mitigation methods for large-scale surveys. Here we present a new RFI mitigation package, called mRAID (multi-beam RAdio frequency Interference Detector), which uses the eigenvalue decomposition algorithm to identify RFI in cross-correlation matrix (CCM) of data recorded by multiple beams. When applied to high time-resolution pulsar search data from the Five-hundred-meter Aperture Spherical Radio Telescope (FAST), mRAID demonstrates excellent performance in identifying RFI over short timescales, thereby enhancing the efficiency of pulsar and fast radio burst (FRB) searches. Since the computation of the CCM and the eigenvalue decomposition for each time sub-integration and frequency channel are independent, the process is fully parallelisable. As a result, mRAID offers a significant computational advantage over commonly used RFI detection methods.

Original languageEnglish
Article numbere008
Number of pages8
JournalPublications of the Astronomical Society of Australia
Volume43
DOIs
Publication statusPublished - 2 Jan 2026

Bibliographical note

Publisher Copyright:
© The Author(s), 2026. Published by Cambridge University Press on behalf of Astronomical Society of Australia.

Keywords

  • methods: data analysis
  • pulsars: general

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