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Updating the First CHIME/FRB Catalog of Fast Radio Bursts with Baseband Data

Authors :
The CHIME/FRB Collaboration
Mandana Amiri
Bridget C. Andersen
Shion Andrew
Kevin Bandura
Mohit Bhardwaj
P. J. Boyle
Charanjot Brar
Daniela Breitman
Tomas Cassanelli
Pragya Chawla
Amanda M. Cook
Alice P. Curtin
Matt Dobbs
Fengqiu Adam Dong
Gwendolyn Eadie
Emmanuel Fonseca
B. M. Gaensler
Utkarsh Giri
Antonio Herrera-Martin
Hans Hopkins
Adaeze L. Ibik
Ronniy C. Joseph
J. F. Kaczmarek
Zarif Kader
Victoria M. Kaspi
Adam E. Lanman
Mattias Lazda
Calvin Leung
Siqi Liu
Kiyoshi W. Masui
Ryan Mckinven
Juan Mena-Parra
Marcus Merryfield
Daniele Michilli
Cherry Ng
Kenzie Nimmo
Gavin Noble
Ayush Pandhi
Chitrang Patel
Aaron B. Pearlman
Ue-Li Pen
Emily Petroff
Ziggy Pleunis
Masoud Rafiei-Ravandi
Mubdi Rahman
Scott M. Ransom
Ketan R. Sand
Paul Scholz
Vishwangi Shah
Kaitlyn Shin
Yuliya Shpunarska
Seth R. Siegel
Kendrick Smith
Ingrid Stairs
David C. Stenning
Keith Vanderlinde
Haochen Wang
Henry White
Dallas Wulf
Source :
The Astrophysical Journal, Vol 969, Iss 2, p 145 (2024)
Publication Year :
2024
Publisher :
IOP Publishing, 2024.

Abstract

In 2021, a catalog of 536 fast radio bursts (FRBs) detected with the Canadian Hydrogen Intensity Mapping Experiment (CHIME) radio telescope was released by the CHIME/FRB Collaboration. This large collection of bursts, observed with a single instrument and uniform selection effects, has advanced our understanding of the FRB population. Here we update the results for 140 of these FRBs for which channelized raw voltage (“baseband”) data are available. With the voltages measured by the telescope’s antennas, it is possible to maximize the telescope sensitivity in any direction within the primary beam, an operation called “beamforming.” This allows us to increase the signal-to-noise ratios of the bursts and to localize them to subarcminute precision. The improved localizations are also used to correct the beam response of the instrument and to measure fluxes and fluences with an ∼10% uncertainty. Additionally, the time resolution is increased by 3 orders of magnitude relative to that in the first CHIME/FRB catalog, and, applying coherent dedispersion, burst morphologies can be studied in detail. Polarization information is also available for the full sample of 140 FRBs, providing an unprecedented data set to study the polarization properties of the population. We release the baseband data beamformed to the most probable position of each FRB. These data are analyzed in detail in a series of accompanying papers.

Details

Language :
English
ISSN :
15384357
Volume :
969
Issue :
2
Database :
Directory of Open Access Journals
Journal :
The Astrophysical Journal
Publication Type :
Academic Journal
Accession number :
edsdoj.66da8275a640459286441a123fa8abcc
Document Type :
article
Full Text :
https://doi.org/10.3847/1538-4357/ad464b