Gamma-ray burst groups observed by BATSE, Beppo-Sax and Swift

I. Horvath; L. G Balazs; Z. Bagoly; P. Veres; D. Szecsi

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arXiv · 1508.04946

Gamma-ray burst groups observed by BATSE, Beppo-Sax and Swift

I. Horvath·L. G Balazs·Z. Bagoly·P. Veres·D. Szecsi

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Abstract

Short and long bursts were identified by the BATSE team in the early 90s. A decade ago there were some suggestions about the intermediate duration type of bursts. We are going to summarize recent analyses of the duration distributions of the Beppo-Sax and Swift data. Our conclusion is all the three satellites (CGRO, Swift, Beppo-Sax) can see the third type of the GRBs. The properties of the group members are very similar in the different data sets.

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I. Horvath, L. G Balazs, Z. Bagoly, P. Veres, D. Szecsi. 2015-08-20. Gamma-ray burst groups observed by BATSE, Beppo-Sax and Swift. https://arxiv.org/abs/1508.04946

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