Verifying Gamma-Ray Burst Duration Analysis Using the Compton Gamma-Ray Observatory T50 Data
arXiv:2608.24507 · doi:10.32562/mkk.2025.2.7
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.
Keywords: gamma-ray burst, gamma-ray, satellites, statistical analysis