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Absolving the SSINS of Precision Interferometric Radio Data: A New Technique for Mitigating Faint Radio Frequency Interference

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arxiv 1906.01093 v3 pith:ZOSH366F submitted 2019-06-03 astro-ph.IM astro-ph.CO

classification astro-ph.IMastro-ph.CO
keywords ssinsdataradioarrayfaintfrequencyinterferencemitigating
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We introduce a new pipeline for analyzing and mitigating radio frequency interference (RFI), which we call Sky-Subtracted Incoherent Noise Spectra (SSINS). SSINS is designed to identify and remove faint RFI below the single baseline thermal noise by employing a frequency-matched detection algorithm on baseline-averaged amplitudes of time-differenced visibilities. We demonstrate the capabilities of SSINS using the Murchison Widefield Array (MWA) in Western Australia. We successfully image aircraft flying over the array via digital television (DTV) reflection detected using SSINS and summarize an RFI occupancy survey of MWA Epoch of Reionization data. We describe how to use SSINS with new data using a documented, publicly available implementation with comprehensive usage tutorials.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. The EDGES Analysis Pipeline: Description and Validation

    astro-ph.IM 2026-05 unverdicted novelty 7.0 of 10

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  2. A Roadmap for Astrophysics and Cosmology with High-Redshift 21 cm Intensity Mapping

    astro-ph.IM 2019-07 unverdicted novelty 2.0 of 10

    A white paper that coordinates a decade-long US program of instrumentation and analysis to enable next-generation 21 cm arrays for cosmology.

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