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We examine the effect of Galactic diffractive interstellar scintillation as a means of explaining the reported deficit of fast radio burst (FRB) detections at low Galactic latitude. We model the unknown underlying FRB flux density distribution as a power law with a rate scaling as $S_\nu ^{-5/2+\delta }$ and account for the fact that the FRBs are detected at unknown positions within the telescope ...

On the paucity of fast radio bursts at low Galactic latitudes