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: http://xray.sai.msu.ru/sciwork/archive/90/eannot2.html
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Before the BATSE/GRO launch GRBs seem to be a uniform phenomenon with duration up to ~100 seconds. The BATSE has detected many events longer than 100 s and a few longer than 500s. We performed the off-line scan of the 1024 ms continuous BATSE records and revealed several non-triggered episodes of the BATSE GRB trigger which confidently belong to the same very long GRBs. There are also several pairs of bursts which are candidates to single very long (''superlong'') GRBs lasting up to ~2000s. Their emission on 500-2000s is prompt emission rather than afterglow. These superlong GRBs probably belong to the class of ''long'' GRBs constituting the tail of their duration distribution. The existence of such events can constrain some models and should be taken into account in the studies of early hard X-ray afterglows. Before BATSE/GRO launch GRBs seem to be a uniform phenomenon with duration up to ~100 seconds. BATSE has detected many events longer than 100 s and a few longer than 500s. We performed the off-line scan of the 1024 ms continuous BATSE records and revealed several non-triggered episodes of the BATSE GRB trigger which confidently belong to the same GRBs. There are also several pairs of bursts which are candidates to single very long (''superlong'') GRBs lasting up to ~2000s. Their emission on 500-2000s is prompt emission rather than afterglow. These superlong GRBs probably belong to the class of ''long'' GRBs constituting the tail of their duration distribution. The existence of such events can constrain some models and should be taken into account in the studies of early hard X-ray afterglows.