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

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arxiv 1508.04946 v1 pith:TN7TJMCQ submitted 2015-08-20 astro-ph.HE

I. Horvath , L.G Balazs , Z. Bagoly , P. Veres , D. Szecsi This is my paper · ORCID
classification astro-ph.HE
keywords beppo-saxswiftbatseburstsdatadurationtypewere
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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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