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The First CHIME/FRB Fast Radio Burst Catalog

Authors :
Collaboration, The CHIME/FRB
Amiri, Mandana
Andersen, Bridget C.
Bandura, Kevin
Berger, Sabrina
Bhardwaj, Mohit
Boyce, Michelle M.
Boyle, P. J.
Brar, Charanjot
Breitman, Daniela
Cassanelli, Tomas
Chawla, Pragya
Chen, Tianyue
Cliche, J. -F.
Cook, Amanda
Cubranic, Davor
Curtin, Alice P.
Deng, Meiling
Dobbs, Matt
Fengqiu
Dong
Eadie, Gwendolyn
Fandino, Mateus
Fonseca, Emmanuel
Gaensler, B. M.
Giri, Utkarsh
Good, Deborah C.
Halpern, Mark
Hill, Alex S.
Hinshaw, Gary
Josephy, Alexander
Kaczmarek, Jane F.
Kader, Zarif
Kania, Joseph W.
Kaspi, Victoria M.
Landecker, T. L.
Lang, Dustin
Leung, Calvin
Li, Dongzi
Lin, Hsiu-Hsien
Masui, Kiyoshi W.
Mckinven, Ryan
Mena-Parra, Juan
Merryfield, Marcus
Meyers, Bradley W.
Michilli, Daniele
Milutinovic, Nikola
Mirhosseini, Arash
Münchmeyer, Moritz
Naidu, Arun
Newburgh, Laura
Ng, Cherry
Patel, Chitrang
Pen, Ue-Li
Petroff, Emily
Pinsonneault-Marotte, Tristan
Pleunis, Ziggy
Rafiei-Ravandi, Masoud
Rahman, Mubdi
Ransom, Scott M.
Renard, Andre
Sanghavi, Pranav
Scholz, Paul
Shaw, J. Richard
Shin, Kaitlyn
Siegel, Seth R.
Sikora, Andrew E.
Singh, Saurabh
Smith, Kendrick M.
Stairs, Ingrid
Tan, Chia Min
Tendulkar, S. P.
Vanderlinde, Keith
Wang, Haochen
Wulf, Dallas
Zwaniga, A. V.
High Energy Astrophys. & Astropart. Phys (API, FNWI)
Source :
Astrophysical Journal, Supplement Series, 257(2):59. IOP Publishing Ltd.
Publication Year :
2021
Publisher :
IOP Publishing Ltd., 2021.

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$^{-3}$.<br />Comment: 67 pages, 27 figures, 5 tables. Published in ApJS and updated with changes reflected in an erratum (affecting the sky rate). Extended figures and data at https://www.chime-frb.ca/catalog

Details

Language :
English
ISSN :
00670049
Volume :
257
Issue :
2
Database :
OpenAIRE
Journal :
The Astrophysical Journal. Supplement Series
Accession number :
edsair.doi.dedup.....609bc4ef2c38cc46dfe227c2ca664c44