Three types of gamma-ray bursts

Mukherjee, Soma, D. Feigelson, Eric, Jogesh Babu, Gutti, Murtagh, Fionn, Fraley, Chris and Raftery, Adrian

(1998)

Mukherjee, Soma, D. Feigelson, Eric, Jogesh Babu, Gutti, Murtagh, Fionn, Fraley, Chris and Raftery, Adrian (1998) Three types of gamma-ray bursts. Astrophysical Journal, 508

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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' $\Lambda^*$ and other MANOVA tests; and a parametric maximum likelihood model-based clustering procedure assuming multinormal populations calculated with the EM Algorithm and validated with the Bayesian Information Criterion. The two methods yield very similar results. The BATSE GRB population consistsof three classes with the following Duration/Fluence/Spectrum bulk properties: Class I with long/bright/intermediate bursts, Class II with short/hard/faintbursts, and Class III with intermediate/intermediate/soft bursts. One outlier with poor data is also present. Classes I and II correspond to those reported by Kouveliotou et al. (1993), but Class III is clearly defined here for the first time.

Information about this Version

This is a Submitted version
This version's date is: 1998
This item is not peer reviewed

Link to this Version

https://repository.royalholloway.ac.uk/items/8a1fd5b3-3d72-1a98-3827-3d79186ae110/5/

Item TypeJournal Article
TitleThree types of gamma-ray bursts
AuthorsMukherjee, Soma
D. Feigelson, Eric
Jogesh Babu, Gutti
Murtagh, Fionn
Fraley, Chris
Raftery, Adrian
Uncontrolled Keywordsastro-ph
DepartmentsFaculty of Science\Computer Science

Identifiers

doihttp://dx.doi.org/10.1086/306386

Deposited by Research Information System (atira) on 22-Jul-2014 in Royal Holloway Research Online.Last modified on 22-Jul-2014

Notes

24 pages, 5 figure, 7 tables. Submitted to the Astrophysical Journal in February 1998


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