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A Third Class of Gamma-Ray Bursts?

© 1998. The American Astronomical Society. All rights reserved. Printed in U.S.A.
, , Citation I. Horváth 1998 ApJ 508 757 DOI 10.1086/306416

0004-637X/508/2/757

Abstract

Two classes of gamma-ray bursts have been identified so far, characterized by T90 durations shorter and longer than approximately 2 s. We show here that the BATSE 3B data allow a good fit with three Gaussian distributions in log T90. The χ2 statistic indicates a 40% probability for two-Gaussian fits, whereas the three-Gaussian fit probability is 98%. Using another statistical method, it is argued that the probability that the third class is a random fluctuation is less than 0.02%.

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10.1086/306416