A Constraint on the Distance Scale to Cosmological Gamma-Ray Bursts

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Abstract
If γ-ray bursts are cosmological in origin, the sources are expected to trace the large-scale structure of luminous matter in the universe. I use a new likelihood method that compares the counts-in-cells distribution of γ-ray bursts in the BATSE 3B catalog with that expected from the known large-scale structure of the universe, in order to place a constraint on the distance scale to cosmological bursts. I find, at the 95% confidence level, that the comoving distance to the "edge" of the burst distribution is greater than 630 h-1 Mpc (z > 0.25), and that the nearest burst is farther than 40 h-1 Mpc. The median distance to the nearest burst is 170 h-1 Mpc, implying that the total energy released in γ-rays during a burst event is of order 3 × 1051 h-2 ergs. None of the bursts that have been observed by BATSE are in nearby galaxies, nor is a signature from the Coma Cluster or the "Great Wall" likely to be seen in the data at present.

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