TY - JOUR
T1 - Radio frequency interference identification using eigenvalue decomposition for multi-beam observations
AU - Bai, Juntao
AU - Dai, Shi
AU - Wang, Na
AU - Osłowski, Stefan
AU - Wang, Shuangqiang
AU - Hobbs, George
AU - Yuan, Jianping
AU - Yan, Wenming
AU - Zhi, Qijun
AU - Shang, Lunhua
AU - Xu, Xin
AU - Dang, Shijun
AU - Zhao, De
N1 - Publisher Copyright:
© The Author(s), 2026. Published by Cambridge University Press on behalf of Astronomical Society of Australia.
PY - 2026/1/2
Y1 - 2026/1/2
N2 - 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.
AB - 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.
KW - methods: data analysis
KW - pulsars: general
UR - http://www.scopus.com/inward/record.url?scp=105026790655&partnerID=8YFLogxK
U2 - 10.1017/pasa.2025.10139
DO - 10.1017/pasa.2025.10139
M3 - Article
AN - SCOPUS:105026790655
SN - 1323-3580
VL - 43
JO - Publications of the Astronomical Society of Australia
JF - Publications of the Astronomical Society of Australia
M1 - e008
ER -