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Mitigating radio frequency interference in CHIME/FRB real-time intensity data

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arxiv 2206.07292 v2 pith:ZFJFN5KN submitted 2022-06-15 astro-ph.IM astro-ph.HE

classification astro-ph.IMastro-ph.HE
keywords radiodatachimeintensityfrbsbandwidthfalsefast
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abstract

Extragalactic fast radio bursts (FRBs) are a new class of astrophysical transients with unknown origins that have become a main focus of radio observatories worldwide. FRBs are highly energetic ($\sim 10^{36}$-$10^{42}$ ergs) flashes that last for about a millisecond. Thanks to its broad bandwidth (400-800 MHz), large field of view ($\sim$200 sq. deg.), and massive data rate (1500 TB of coherently beamformed data per day), the Canadian Hydrogen Intensity Mapping Experiment / Fast Radio Burst (CHIME/FRB) project has increased the total number of discovered FRBs by over a factor 10 in 3 years of operation. CHIME/FRB observations are hampered by the constant exposure to radio frequency interference (RFI) from artificial devices (e.g., cellular phones, aircraft), resulting in $\sim$20% loss of bandwidth. In this work, we describe our novel technique for mitigating RFI in CHIME/FRB real-time intensity data. We mitigate RFI through a sequence of iterative operations, which mask out statistical outliers from frequency-channelized intensity data that have been effectively high-pass filtered. Keeping false positive and false negative rates at very low levels, our approach is useful for any high-performance surveys of radio transients in the future.

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Cited by 1 Pith paper

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  1. Energy and polarization based on-line interference mitigation in radio interferometry

    astro-ph.IM 2024-12 conditional novelty 6.0 of 10

    Combining spectral kurtosis with polarization alignment enables real-time RFI flagging in correlators, and RL-tuned mixed precision matches full precision within 1%.

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