Verifying Gamma-Ray Burst Duration Analysis Using the Compton Gamma-Ray Observatory T50 Data

arXiv:2608.24507 · astro-ph.HE · Submitted 2026-07-24 · Read on arXiv

astro-ph.HE

Submitted: 2026-07-24

Updated: 2026-07-24

Comments: Keywords: gamma-ray burst, gamma-ray, satellites, statistical analysis

Journal ref: Muszaki Katonai Kozlony 35 : 2 pp. 97-106. 10 p. (2025)

DOI: 10.32562/mkk.2025.2.7

License: http://creativecommons.org/licenses/by-nc-nd/4.0/

The gist: Several authors have shown in the literature that a third type of gamma-ray burst class can be detected in the Compton Gamma-Ray Observatory data using T90.

Abstract

Several authors have shown in the literature that a third type of gamma-ray burst class can be detected in the Compton Gamma-Ray Observatory data using T90. In this paper, I examine whether this can also be found in the T50 variable data from the Compton Gamma-Ray Observatory Burst And Transient Source Experiment observation. According to my calculations, the third group detected in T90 can also be detected in the T50 data.

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