The spatial distribution of gamma-ray bursts from Pioneer Venus Orbiter

Mathematics – Probability

Scientific paper

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Gamma Ray Bursts, Pioneer Venus 1 Spacecraft, Spatial Distribution, Background Radiation, Least Squares Method, Radiation Detectors, Statistical Analysis

Scientific paper

The homogeneity of the burst source population in space with the log N(greater than Pc)-log Pc and log (dN/dPc)-log Pc relations is studied on the basis of a sample of 225 observed gamma-ray bursts between September 1978 and July 1988 from the Pioneer Venus Orbiter. The relations N(greater than Pc) is approximately equal to Pc exp -1.5 and dN/dPc is approximately equal to Pc exp -2.5 are expected if the gamma bursters are uniformly distributed in space. The Kolmogorov-Smirnov statistic gives a probability of 0.93 that the observed integral distribution N(greater than Pc) is drawn from the expected uniform distribution Pc exp -1.5. A least-squares 1 standard deviation fit to the observed differential distribution yields dN/dPc of about Pc -2.42 +/- 0.07. Both are consistent with a uniform distribution in space of the parent population of burst sources.

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