CHIME/FRB Discovery of 25 Repeating Fast Radio Burst Sources
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Published:2023-04-01
Issue:2
Volume:947
Page:83
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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:
The CHIME/FRB Collaboration , Andersen Bridget C.ORCID, Bandura KevinORCID, Bhardwaj MohitORCID, Boyle P. J.ORCID, Brar CharanjotORCID, Cassanelli TomasORCID, Chatterjee S.ORCID, Chawla PragyaORCID, Cook Amanda M.ORCID, Curtin Alice P.ORCID, Dobbs MattORCID, Dong Fengqiu AdamORCID, Faber Jakob T.ORCID, Fandino MateusORCID, Fonseca EmmanuelORCID, Gaensler B. M.ORCID, Giri UtkarshORCID, Herrera-Martin AntonioORCID, Hill Alex S.ORCID, Ibik AdaezeORCID, Josephy AlexanderORCID, Kaczmarek Jane F.ORCID, Kader ZarifORCID, Kaspi VictoriaORCID, Landecker T. L.ORCID, Lanman Adam E.ORCID, Lazda MattiasORCID, Leung CalvinORCID, Lin Hsiu-HsienORCID, Masui Kiyoshi W.ORCID, Mckinven RyanORCID, Mena-Parra JuanORCID, Meyers Bradley W.ORCID, Michilli D.ORCID, Ng CherryORCID, Pandhi AyushORCID, Pearlman Aaron B.ORCID, Pen Ue-LiORCID, Petroff EmilyORCID, Pleunis ZiggyORCID, Rafiei-Ravandi MasoudORCID, Rahman MubdiORCID, Ransom Scott M.ORCID, Renard AndreORCID, Sand Ketan R.ORCID, Sanghavi PranavORCID, Scholz PaulORCID, Shah VishwangiORCID, Shin KaitlynORCID, Siegel SethORCID, Smith KendrickORCID, Stairs IngridORCID, Su JianingORCID, Tendulkar Shriharsh P.ORCID, Vanderlinde KeithORCID, Wang HaochenORCID, Wulf DallasORCID, Zwaniga AndrewORCID
Abstract
Abstract
We present the discovery of 25 new repeating fast radio burst (FRB) sources found among CHIME/FRB events detected between 2019 September 30 and 2021 May 1. The sources were found using a new clustering algorithm that looks for multiple events colocated on the sky having similar dispersion measures (DMs). The new repeaters have DMs ranging from ∼220 to ∼1700 pc cm−3, and include sources having exhibited as few as two bursts to as many as twelve. We report a statistically significant difference in both the DM and extragalactic DM (eDM) distributions between repeating and apparently nonrepeating sources, with repeaters having a lower mean DM and eDM, and we discuss the implications. We find no clear bimodality between the repetition rates of repeaters and upper limits on repetition from apparently nonrepeating sources after correcting for sensitivity and exposure effects, although some active repeating sources stand out as anomalous. We measure the repeater fraction over time and find that it tends to an equilibrium of
2.6
−
2.6
+
2.9
% over our total time-on-sky thus far. We also report on 14 more sources, which are promising repeating FRB candidates and which merit follow-up observations for confirmation.
Funder
Canada Foundation for Innovation National Science Foundation Gouvernement du Canada ∣ Natural Sciences and Engineering Research Council of Canada
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Cited by
46 articles.
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