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  5. Two Dimensional Clustering of Swift/BAT and Fermi/GBM Gamma-ray Bursts
 
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Two Dimensional Clustering of Swift/BAT and Fermi/GBM Gamma-ray Bursts

Author(s)
Salmon, Lana  
Hanlon, Lorraine  
Martin-Carrillo, Antonio  
Uri
http://hdl.handle.net/10197/13037
Date Issued
2022-06-25
Date Available
2022-08-05T08:44:57Z
Abstract
Studies of Gamma-ray Burst (GRB) properties, such as duration and spectral hardness, have found evidence for additional classes beyond the short-hard (merger) and long-soft (collapsar) prototypes. Several clustering analyses of the duration-hardness plane identified a third, intermediate duration, class. In this work, Gaussian Mixture Model-based (GMM) clustering is applied to the Swift/BAT and Fermi/GBM samples of GRBs. The results obtained by the hierarchical combination of Gaussian components (or clusters) based on an entropy criterion are presented. This method counteracts possible overfitting arising from the application of Gaussian models to non-Gaussian underlying data. While the initial GMM clustering of the hardness-duration plane identifies three components (short/intermediate/long) for the Swift/BAT and Fermi/GBM samples, only two components (short/long) remain once the entropy criterion is applied. The analysis presented here suggests that the intermediate duration class may be the result of overfitting, rather than evidence of a distinct underlying population.
Sponsorship
European Commission Horizon 2020
Science Foundation Ireland
Other Sponsorship
Irish Research Council Postgraduate Scholarship
Type of Material
Journal Article
Publisher
MDPI
Journal
Galaxies
Volume
10
Issue
4
Start Page
1
End Page
17
Copyright (Published Version)
2022 The Authors
Subjects

Gamma-ray burst

Clustering

Statistical analysis

DOI
10.3390/galaxies10040077
Language
English
Status of Item
Peer reviewed
ISSN
2075-4434
This item is made available under a Creative Commons License
https://creativecommons.org/licenses/by/3.0/ie/
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Clustering_250622.pdf

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647.77 KB

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Checksum (MD5)

21e722a8d0eb83f24580b1413bc2e89b

Owning collection
Physics Research Collection

Item descriptive metadata is released under a CC-0 (public domain) license: https://creativecommons.org/public-domain/cc0/.
All other content is subject to copyright.

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