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A Real-time Single Pulse Detection Algorithm for GPUs

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arxiv 1611.09704 v1 pith:O5FUVTIZ submitted 2016-11-29 astro-ph.IM

classification astro-ph.IM
keywords codealgorithmdetectionpulseradiosingleastroaccelerateastronomy
verification ladder T0 review T1 audit T2 compute T3 formal
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The detection of non-repeating events in the radio spectrum has become an important area of study in radio astronomy over the last decade due to the discovery of fast radio bursts (FRBs). We have implemented a single pulse detection algorithm, for NVIDIA GPUs, which use boxcar filters of varying widths. Our code performs the calculation of standard deviation, matched filtering by using boxcar filters and thresholding based on the signal-to-noise ratio. We present our parallel implementation of our single pulse detection algorithm. Our GPU algorithm is approximately 17x faster than our current CPU OpenMP code (NVIDIA Titan XP vs Intel E5-2650v3). This code is part of the AstroAccelerate project which is a many-core accelerated time-domain signal processing code for radio astronomy. This work allows our AstroAccelerate code to perform a single pulse search on SKA-like data 4.3x faster than real-time.

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Cited by 1 Pith paper

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

  1. Contemporaneous optical-radio observations of a fast radio burst in a close galaxy pair

    astro-ph.HE 2025-02 conditional novelty 5.0 of 10

    A new fast radio burst was caught with an optical follow-up image starting 3.4 s later, giving a fluence ratio limit F_opt/F_radio <= 0.023 for a non-repeater.

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