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Morphology of 137 Fast Radio Bursts down to Microseconds Timescales from The First CHIME/FRB Baseband Catalog

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arxiv 2408.13215 v1 pith:BBSAP3QV submitted 2024-08-23 astro-ph.HE

classification astro-ph.HE
keywords burstssamplecatalogchimecomponentsfirstfrbsmeasure
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abstract

We present a spectro-temporal analysis of 137 fast radio bursts (FRBs) from the first CHIME/FRB baseband catalog, including 125 one-off bursts and 12 repeat bursts, down to microsecond resolution using the least-squares optimization fitting routine: fitburst. Our measured values are compared with those in the first CHIME/FRB intensity catalog, revealing that nearly one-third of our sample exhibits additional burst components at higher time resolutions. We measure sub-burst components within burst envelopes as narrow as $\sim$23 $\mu$s (FWHM), with 20% of the sample displaying sub-structures narrower than 100 $\mu$s, offering constraints on emission mechanisms. Scattering timescales in the sample range from 30 $\mu$s to 13 ms at 600 MHz. We observe no correlations between scattering time and dispersion measure, rotation measure, or linear polarization fraction, with the latter suggesting that depolarization due to multipath propagation is negligible in our sample. Bursts with narrower envelopes ($\leq$ 1 ms) in our sample exhibit higher flux densities, indicating the potential presence of sub-ms FRBs that are being missed by our real-time system below a brightness threshold. Most multicomponent bursts in our sample exhibit sub-burst separations of $\leq$ 1 ms, with no bursts showing separations $<$41 $\mu$s, even at a time resolution of 2.56 $\mu$s, but both scattering and low signal-to-noise ratio can hinder detection of additional components. Lastly, given the morphological diversity of our sample, we suggest that one-off and repeating FRBs can come from different classes but have overlapping property distributions.

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Cited by 4 Pith papers

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

  1. Detection of Partial Coherence due to Multipath Propagation for FRB 20220413B with CHIME/FRB

    astro-ph.HE 2025-12 conditional novelty 6.0 of 10

    FRB 20220413B's components share a common Milky Way scintillation pattern but show no phase-coherent lensing signature, so the complex morphology is not confirmed as plasma lensing.

  2. A Unified Volumetric Rate-Energy Relation from Magnetar Radio Bursts to Fast Radio Bursts

    astro-ph.HE 2025-07 conditional novelty 6.0 of 10

    The volumetric rate of radio bursts from magnetar SGR 1935+2154, repeating FRB 20180916B, and non-repeating CHIME FRBs follows a single power law R ∝ E^-1.31 from 10^29 to 10^42 erg.

  3. Discovery and Localization of the Swift-Observed FRB 20241228A in a Star-forming Host Galaxy

    astro-ph.HE 2025-06 conditional novelty 6.0 of 10

    FRB 20241228A is localized to a star-forming galaxy at z=0.1614, with a stringent X-ray limit from Swift follow-up 112 seconds after the burst.

  4. Semi-supervised morphological classification of fast radio bursts from the second CHIME/FRB catalogue

    astro-ph.HE 2026-07 conditional novelty 5.0 of 10

    A simulation-trained convolutional autoencoder identifies three distinct FRB morphological classes and classifies repeatability with 86% recall.

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