Updating the First CHIME/FRB Catalog of Fast Radio Bursts with Baseband Data
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Published:2024-07-01
Issue:2
Volume:969
Page:145
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ISSN:0004-637X
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Container-title:The Astrophysical Journal
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language:
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Short-container-title:ApJ
Author:
, Amiri MandanaORCID, Andersen Bridget C.ORCID, Andrew ShionORCID, Bandura KevinORCID, Bhardwaj MohitORCID, Boyle P. J.ORCID, Brar CharanjotORCID, Breitman DanielaORCID, Cassanelli TomasORCID, Chawla PragyaORCID, Cook Amanda M.ORCID, Curtin Alice P.ORCID, Dobbs MattORCID, Dong Fengqiu AdamORCID, Eadie GwendolynORCID, Fonseca EmmanuelORCID, Gaensler B. M.ORCID, Giri UtkarshORCID, Herrera-Martin AntonioORCID, Hopkins HansORCID, Ibik Adaeze L.ORCID, Joseph Ronniy C.ORCID, Kaczmarek J. F.ORCID, Kader ZarifORCID, Kaspi Victoria M.ORCID, Lanman Adam E.ORCID, Lazda MattiasORCID, Leung CalvinORCID, Liu SiqiORCID, Masui Kiyoshi W.ORCID, Mckinven RyanORCID, Mena-Parra JuanORCID, Merryfield MarcusORCID, Michilli DanieleORCID, Ng CherryORCID, Nimmo KenzieORCID, Noble GavinORCID, Pandhi AyushORCID, Patel ChitrangORCID, Pearlman Aaron B.ORCID, Pen Ue-LiORCID, Petroff EmilyORCID, Pleunis ZiggyORCID, Rafiei-Ravandi MasoudORCID, Rahman MubdiORCID, Ransom Scott M.ORCID, Sand Ketan R.ORCID, Scholz PaulORCID, Shah VishwangiORCID, Shin KaitlynORCID, Shpunarska YuliyaORCID, Siegel Seth R.ORCID, Smith KendrickORCID, Stairs IngridORCID, Stenning David C.ORCID, Vanderlinde KeithORCID, Wang HaochenORCID, White HenryORCID, Wulf DallasORCID
Abstract
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.
Publisher
American Astronomical Society
Cited by
1 articles.
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