Rising indications for three gamma-ray burst groups
J. Ripa, D. Huja, A. Meszaros, C. Wigger
TL;DR
This paper investigates the existence of three distinct groups of gamma-ray bursts using statistical analysis of their durations and hardness ratios from Swift and RHESSI datasets.
Contribution
It provides new statistical evidence supporting the classification of GRBs into three groups based on recent satellite data.
Findings
Identification of three gamma-ray burst groups
Distinct statistical properties for each group
Enhanced understanding of GRB classification
Abstract
Several papers were written about the gamma-ray burst (GRBs) groups. Our statistical study is based on the durations and hardness ratios of the Swift and RHESSI data.
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Taxonomy
TopicsGamma-ray bursts and supernovae