Latent characterization of the complete BATSE gamma-ray bursts catalogue using Gaussian mixture of factor analysers and model-estimated overlap-based syncytial clustering

ABSTRACT Characterizing and distinguishing gamma-ray bursts (GRBs) has interested astronomers for many decades. While some authors have found two or three groups of GRBs by analysing only a few parameters, recent work identified five ellipsoidally shaped groups upon considering nine parameters $T_{50}, T_{90}, F_1, F_2, F_3, F_4, P_{64}, P_{256}, P_{1024}$. Yet others suggest subclasses within the two or three groups found earlier. Using a mixture model of Gaussian factor analysers, we analysed 1150 GRBs, that had nine parameters observed, from the current Burst and Transient Source Experiment (BATSE) catalogue, and again established five ellipsoidal-shaped groups to describe the GRBs. These five groups are characterized in terms of their average duration, fluence, and spectrum as shorter-faint-hard, long-intermediate-soft, long-intermediate-intermediate, long-bright-intermediate, and short-faint-hard. The use of factor analysers in describing individual group densities allows for a more thorough group-wise characterization of the parameters in terms of a few latent features. However, given the discrepancy with many other existing studies that advocated for two or three groups, we also performed model-estimated overlap-based syncytial clustering that successively merges poorer separated groups. The five ellipsoidal groups merge into three and then into two groups, one with GRBs of low durations and the other having longer duration GRBs. These groups are also characterized in terms of a few latent factors made up of the nine parameters. Our analysis provides context for all three sets of results, and in doing so, details a multilayered characterization of the BATSE GRBs, while also explaining the structure in their variability.

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Publication Details

Journal
Monthly Notices of the Royal Astronomical Society
Published
2024-11-12
DOI
https://doi.org/10.1093/mnras/stae2548
Citations
2
Primary Topic
Gamma-ray bursts and supernovae
Type
article
Field-Weighted Citation Impact
0.66
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article

Latent characterization of the complete BATSE gamma-ray bursts catalogue using Gaussian mixture of factor analysers and model-estimated overlap-based syncytial clustering

Ranjan Maitra, Fan Dai
2 citations
Monthly Notices of the Royal Astronomical Society
Gamma-ray bursts and supernovae
0.66
article

Latent characterization of the complete BATSE gamma-ray bursts catalogue using Gaussian mixture of factor analysers and model-estimated overlap-based syncytial clustering

Ranjan Maitra, Fan Dai
article en
2 citations

Abstract

ABSTRACT Characterizing and distinguishing gamma-ray bursts (GRBs) has interested astronomers for many decades. While some authors have found two or three groups of GRBs by analysing only a few parameters, recent work identified five ellipsoidally shaped groups upon considering nine parameters $T_{50}, T_{90}, F_1, F_2, F_3, F_4, P_{64}, P_{256}, P_{1024}$. Yet others suggest subclasses within the two or three groups found earlier. Using a mixture model of Gaussian factor analysers, we analysed 1150 GRBs, that had nine parameters observed, from the current Burst and Transient Source Experiment (BATSE) catalogue, and again established five ellipsoidal-shaped groups to describe the GRBs. These five groups are characterized in terms of their average duration, fluence, and spectrum as shorter-faint-hard, long-intermediate-soft, long-intermediate-intermediate, long-bright-intermediate, and short-faint-hard. The use of factor analysers in describing individual group densities allows for a more thorough group-wise characterization of the parameters in terms of a few latent features. However, given the discrepancy with many other existing studies that advocated for two or three groups, we also performed model-estimated overlap-based syncytial clustering that successively merges poorer separated groups. The five ellipsoidal groups merge into three and then into two groups, one with GRBs of low durations and the other having longer duration GRBs. These groups are also characterized in terms of a few latent factors made up of the nine parameters. Our analysis provides context for all three sets of results, and in doing so, details a multilayered characterization of the BATSE GRBs, while also explaining the structure in their variability.

Monthly Notices of the Royal Astronomical SocietyVol. 535(4)
Michigan Technological University (US), Iowa State University (US)
No poverty
Openalex Percentile: Top 27%
Gamma-ray bursts and supernovae
0.66
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