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Gravitational lensing probability for the Konus-Wind gamma-ray bursts detected in the triggered mode
Author(s) -
A. Tsvetkova,
D. Svinkin,
D. Frederiks
Publication year - 2019
Publication title -
journal of physics. conference series
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 0.21
H-Index - 85
eISSN - 1742-6596
pISSN - 1742-6588
DOI - 10.1088/1742-6596/1400/2/022043
Subject(s) - gamma ray burst , astrophysics , physics , gravitational lens , redshift , luminosity function , luminosity , event (particle physics) , astronomy , galaxy
Although half a century has passed since the discovery of Gamma-ray bursts (GRBs), there is no evidence for any strongly lensed event. Using GRB luminosity function and GRB formation rate estimates for the Konus-Wind burst sample with known redshifts, and a Singular Isothermal Sphere as a gravitational lens model, we predict the detection rate of both GRB images being ≈ 0.02–0.05 events per year. The result is consistent with the non-detection of lensed bursts in the KW triggered GRB sample.

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