The Rate of Short-Duration Gamma-Ray Bursts in the Local Universe
arXiv:1812.00507 · doi:10.3390/galaxies6040130
Abstract
Following the faint gamma-ray burst, GRB 170817A, coincident with a gravitational wave-detected binary neutron star merger at Mpc, we consider the constraints on a local population of faint short duration GRBs (defined here broadly as s). We review proposed low-redshift short-GRBs and consider statistical limits on a Mpc population using Swift/Burst Alert Telescope (BAT), Fermi/Gamma-ray Burst Monitor (GBM), and Compton Gamma-Ray Observatory (CGRO) Burst and Transient Source Experiment (BATSE) GRBs. Swift/BAT short-GRBs give an upper limit for the all-sky rate of y at Mpc, corresponding to % of SGRBs. Cross-correlation of selected CGRO/BATSE and Fermi/GBM GRBs with Mpc galaxy positions returns a weaker constraint of . A separate search for correlations due to SGR giant flares in nearby ( Mpc) galaxies finds an upper limit of . Our analysis suggests that GRB 170817A-like events are likely to be rare in existing SGRB catalogues. The best candidate for an analogue remains GRB 050906, where the Swift/BAT location was consistent with the galaxy IC0327 at Mpc. If binary neutron star merger rates are at the high end of current estimates, then our results imply that at most a few percent will be accompanied by detectable gamma-ray flashes in the forthcoming LIGO/Virgo science runs.
arXiv comment16 pages, 4 figures, 1 table. Published in Galaxies as part of the Special Issue, "Observations and Theory of Short GRBs at the Dawn of the Gravitational Wave Era"
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