Document Type
Article
Publication Date
1-1-1998
Abstract
A multivariate analysis of gamma-ray burst (GRB) bulk properties is presented to discriminate between distinct classes of GRBs. Several variables representing burst duration, fluence, and spectral hardness are considered. Two multivariate clustering procedures are used on a sample of 797 bursts from the Third BATSE Catalog, a nonparametric average linkage hierarchical agglomerative clustering procedure validated with Wilks' Λ* and other multivariate analysis of variance tests and a parametric maximum likelihood model-based clustering procedure assuming multinormal populations calculated with the Expectation-Maximization algorithm and validated with the Bayesian Information Criterion. The two methods yield very similar results. The BATSE GRB population consists of three classes with the following duration/fluence/spectrum bulk properties: class I with long/bright/soft bursts, class II with short/faint/hard bursts, and class III with intermediate/intermediate/soft bursts. One outlier due to spurious data is also present. Classes I and II correspond to those reported by Kouveliotou et al., but class III is clearly defined here for the first time. © 1998. The American Astronomical Society. All rights reserved.
Recommended Citation
Soma Mukherjee, et. al., (1998) Three types of gamma-ray bursts.Astrophysical Journal508:1314. DOI: http://doi.org/10.1086/306386
First Page
314
Last Page
327
Publication Title
Astrophysical Journal
DOI
10.1086/306386
Comments
© Astrophysical Journal. Original version available at: http://doi.org/10.1086/306386