pith. sign in

arxiv: 2106.04352 · v3 · pith:GWXA5D7Dnew · submitted 2021-06-08 · 🌌 astro-ph.HE · astro-ph.CO· astro-ph.IM

The First CHIME/FRB Fast Radio Burst Catalog

classification 🌌 astro-ph.HE astro-ph.COastro-ph.IM
keywords textrmburstspopulationcatalogchimeeventsfastnon-repeaters
0
0 comments X
read the original abstract

We present a catalog of 536 fast radio bursts (FRBs) detected by the Canadian Hydrogen Intensity Mapping Experiment Fast Radio Burst (CHIME/FRB) Project between 400 and 800 MHz from 2018 July 25 to 2019 July 1, including 62 bursts from 18 previously reported repeating sources. The catalog represents the first large sample, including bursts from repeaters and non-repeaters, observed in a single survey with uniform selection effects. This facilitates comparative and absolute studies of the FRB population. We show that repeaters and apparent non-repeaters have sky locations and dispersion measures (DMs) that are consistent with being drawn from the same distribution. However, bursts from repeating sources differ from apparent non-repeaters in intrinsic temporal width and spectral bandwidth. Through injection of simulated events into our detection pipeline, we perform an absolute calibration of selection effects to account for systematic biases. We find evidence for a population of FRBs - comprising a large fraction of the overall population - with a scattering time at 600 MHz in excess of 10 ms, of which only a small fraction are observed by CHIME/FRB. We infer a power-law index for the cumulative fluence distribution of $\alpha=-1.40\pm0.11(\textrm{stat.})^{+0.06}_{-0.09}(\textrm{sys.})$, consistent with the $-3/2$ expectation for a non-evolving population in Euclidean space. We find $\alpha$ is steeper for high-DM events and shallower for low-DM events, which is what would be expected when DM is correlated with distance. We infer a sky rate of $[525\pm30(\textrm{stat.})^{+140}_{-130}({\textrm{sys.}})]/\textrm{sky}/\textrm{day}$ above a fluence of 5 Jy ms at 600 MHz, with scattering time at $600$ MHz under 10 ms, and DM above 100 pc cm$^{-3}$.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.

Forward citations

Cited by 10 Pith papers

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

  1. Dispersion Measure Distribution of Unlocalized Fast Radio Bursts as a Probe of the Hubble Constant

    astro-ph.CO 2026-04 unverdicted novelty 8.0

    The DM distribution of unlocalized FRBs yields H0 = 73.8 +14.0/-12.3 km/s/Mpc with 18% uncertainty.

  2. Gravitational Gertsenshtein-Zeldovich mechanism for the Association between GW190425 and FRB 20190425A

    astro-ph.HE 2026-04 unverdicted novelty 7.0

    Kilohertz gravitational waves from a neutron star merger convert to electromagnetic waves near a magnetar via the Gertsenshtein-Zeldovich effect and are inverse Compton scattered to gigahertz frequencies to explain th...

  3. Fast Radio Burst Dispersion Measure--Timing Cross-Correlations: Bias Self-Calibration and Primordial Non-Gaussianity Constraints

    astro-ph.CO 2026-04 unverdicted novelty 7.0

    DM-Shapiro timing cross-correlations self-calibrate electron bias b_e, recovering sigma(f_NL) within 1.0-1.9 of fixed-bias performance after marginalization.

  4. Generalized Distributions of Host Dispersion Measures in the Fast Radio Burst Cosmology

    astro-ph.CO 2025-10 unverdicted novelty 6.0

    Generalizing the host galaxy dispersion measure distribution in FRB cosmology with 125 events produces Hubble constant estimates consistent with Planck 2018 and SH0ES while strongly favoring these models over narrow-p...

  5. Radio Emission from High-Frequency Gravitational Wave Point Sources

    hep-ph 2026-06 unverdicted novelty 5.0

    Radio telescopes outperform other experiments at detecting high-frequency gravitational waves from primordial black hole mergers and boson clouds through conversion to radio signals in magnetic fields.

  6. Simulating FRB Morphologies and Coherent Phase Correlation Signatures from Multi-Plane Astrophysical Lensing

    astro-ph.HE 2024-07 unverdicted novelty 5.0

    Simulation tool for multi-plane lensing of FRB point sources using coherent geometric optics on a spatial grid to produce morphologies and phase correlation signatures.

  7. The impact of FRB dispersion measure probability distribution functions on cosmographic estimates

    astro-ph.CO 2026-06 unverdicted novelty 4.0

    Cosmographic constraints from 106 FRBs on H0, q0, j0 depend sensitively on whether a Gaussian or quasi-Gaussian PDF is assumed for DM_IGM and on whether the baryon mass fraction is fixed or free.

  8. Probing Primordial Black Holes with upcoming Radio Telescopes: a case study for LOFAR2.0, FAST Core Array and BINGO

    astro-ph.CO 2026-04 unverdicted novelty 4.0

    LOFAR2.0, FAST Core Array and BINGO can constrain the PBH dark matter fraction f_PBH below 0.16-0.39 for masses above 10^{-2} to 10 solar masses via FRB lensing statistics.

  9. MUltiplexed Survey Telescope (MUST) Science White Paper I: Overview of Large-Scale Structure Cosmology in the Era of Stage-V Spectroscopic Surveys

    astro-ph.CO 2024-11 unverdicted novelty 4.0

    MUST is a planned 6.5m Stage-V spectroscopic survey telescope targeting 100M+ galaxies and quasars to z~5.5 for large-scale structure cosmology studies.

  10. Fast Radio Bursts as Cosmological Probes

    astro-ph.CO 2026-06 unverdicted novelty 2.0

    FRBs serve as cosmological probes via dispersion measure, scattering, and Faraday rotation to constrain baryon distribution, expansion history, magnetic fields, and fundamental physics effects.