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Statistical analysis of the prompt and afterglow emission of the three groups of gamma-ray bursts

We investigated the main prompt and afterglow emission parameters of gamma-ray bursts detected by the Burst Alert Telescope (BAT) and X-Ray Telescope installed on the Swift satellite. Our aim was to look for differences or connections between the different types of gamma-ray bursts, so we compared the BAT fluences, 1-sec peak photon fluxes, photon indices, XRT early fluxes, initial temporal decay and spectral indices. We found that there might be a connection between the XRT initial decay index and XRT early flux/BAT photon index. Using statistical tools we also determined that beside the duration and hardness ratios, the means of the γ- and X-ray--fluences and the γ-ray photon index differ significantly between the three types of bursts.

preprint2013arXivOpen access
J. KóboriZ. BagolyL. G. BalázsI. Horváth
astro-ph.HE
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J. KóboriZ. BagolyL. G. BalázsI. Horváth

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