2024MNRAS.52711158Y


Query : 2024MNRAS.52711158Y

2024MNRAS.52711158Y - Mon. Not. R. Astron. Soc., 527, 11158-11166 (2024/February-1)

The true fraction of repeating fast radio bursts revealed through CHIME source count evolution.

YAMASAKI S., GOTO T., LING C.-T. and HASHIMOTO T.

Abstract (from CDS):

Fast Radio Bursts (FRBs) are classified into repeaters and non-repeaters, with only a few per cent of the observed FRB population from the Canadian Hydrogen Intensity Mapping Experiment (CHIME) confirmed as repeaters. However, this figure represents only a lower limit due to the observational biases, and the true fraction of repeaters remains unknown. Correcting for these biases uncovers a notable decline in apparently non-repeating FRB detection rate as the CHIME operational time increases. This finding suggests that a significant portion of apparently non-repeating FRBs could in fact exhibit repetition when observed over more extended periods. A simple population model infers that the true repeater fraction likely exceeds 50 per cent with 99 per cent confidence, a figure substantially larger than the observed face value, even consistent with 100 per cent. This greater prevalence of repeaters had previously gone unnoticed due to their very low repetition rates (∼10–3.5 h–1 on average). Hence, theoretical FRB models must incorporate these low-rate repeaters. Furthermore, our results indicate a significantly higher repeater volume number density, potentially exceeding observed values by up to 104 times, which in turn impacts comparisons with potential FRB progenitors.

Abstract Copyright: © The Author(s) 2023. Published by Oxford University Press on behalf of Royal Astronomical Society.

Journal keyword(s): radio continuum: transients - fast radio bursts

Simbad objects: 1

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Number of rows : 1
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 FRB 20180916B rB 01 58 00.750 +65 43 00.30           ~ 457 0

Query : 2024MNRAS.52711158Y

Basic data :
FRB 20180916B -- Radio Burst
Other object types:
otypes_help
rB (2021ApJS,FRB), Rad (2019ApJ), ev (AT)
ICRS coord. (ep=J2000) :
01 58 00.750 +65 43 00.30 (Radio) [ ] E 2022ApJ...929..139L
FK4 coord. (ep=B1950 eq=1950) :
01 54 15.539 +65 28 24.27 [ ]
Gal coord. (ep=J2000) :
129.710827 +03.725027 [ ]
Radial velocity / Redshift / cz :
V(km/s) 9933 [60] / z(~) 0.0337 [0.0002] / cz 10103 [60]
   D 2020Natur.577..190M
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Hierarchy : number of linked objects
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Identifiers (25) :
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NAME FRB 180916.J0158+65 FRB 20190126A FRB 20190605B FRB 20181019A
AT 2020hur FRB 20181225A FRB 20190604F FRB 20180916B
FRB 20190605A FRB 20181120B FRB 20190519B FRB 220908
FRB 20190603A FRB 20181104B FRB 20190519A FRB 20210320A
FRB 20190519C FRB 20181104A FRB 20181226A
FRB 20190518E FRB 18090106B FRB 20181223A
FRB 20190518A FRB 180916 FRB 20181222A

References (457 between 1850 and 2026) (Total 457)
Simbad bibliographic survey began in 1850 for stars (at least bright stars) and in 1983 for all other objects (outside the solar system).
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