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Fast Radio Burst 121102 Pulse Detection and Periodicity: A Machine Learning Approach

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arxiv 1809.03043 v1 pith:OVODZJY7 submitted 2018-09-09 astro-ph.HE astro-ph.IM

Fast Radio Burst 121102 Pulse Detection and Periodicity: A Machine Learning Approach

classification astro-ph.HE astro-ph.IM
keywords pulsesdetectionpulseperiodicitytimearrivalsburstdata
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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We report the detection of 72 new pulses from the repeating fast radio burst FRB 121102 in Breakthrough Listen C-band (4-8 GHz) observations at the Green Bank Telescope. The new pulses were found with a convolutional neural network in data taken on August 26, 2017, where 21 bursts have been previously detected. Our technique combines neural network detection with dedispersion verification. For the current application we demonstrate its advantage over a traditional brute-force dedis- persion algorithm in terms of higher sensitivity, lower false positive rates, and faster computational speed. Together with the 21 previously reported pulses, this observa- tion marks the highest number of FRB 121102 pulses from a single observation, total- ing 93 pulses in five hours, including 45 pulses within the first 30 minutes. The number of data points reveal trends in pulse fluence, pulse detection rate, and pulse frequency structure. We introduce a new periodicity search technique, based on the Rayleigh test, to analyze the time of arrivals, with which we exclude with 99% confidence pe- riodicity in time of arrivals with periods larger than 5.1 times the model-dependent time-stamp uncertainty. In particular, we rule out constant periods >10 ms in the barycentric arrival times, though intrinsic periodicity in the time of emission remains plausible.

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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. Depolarization Induced by Rapid Polarization Angle Swings: A Common Feature of Pulsars and Fast Radio Bursts?

    astro-ph.HE 2026-07 conditional novelty 6.0

    Rapid polarization-angle swings should depolarize pulsar and FRB emission, yielding an anti-correlation Π_L vs dPA/dt that has tentative support in a subset of pulsars.

  2. Signatures of Two Distinct Epochs of FRB 20240114A from January to August 2024 Based on its Energy and Waiting Time Analysis

    astro-ph.HE 2026-07 unverdicted novelty 4.0

    FRB 20240114A shows two epochs with distinct energy distribution indices and waiting time statistics, suggesting different burst types before and after March 21 2024.