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Short and long bursts were identified by the BATSE team in the early 90s. Adecade ago there were some suggestions about the intermediate duration type ofbursts. We are going to summarize recent analyses of the duration distributionsof 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 ofthe group members are very similar in the different data sets.

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