Gamma‐ray bursts are usually classified through their high‐energy emission into short‐duration and long‐duration bursts. A third intermediate group has been identified on statistical grounds but its individual pro...
Gamma‐ray bursts are usually classified through their high‐energy emission into short‐duration and long‐duration bursts. A third intermediate group has been identified on statistical grounds but its individual properties have not yet been studied in detail. Using the large sample of follow‐up observations of GRBs produced during the Swift era we analyze the individual characteristics of this group. We find that intermediate bursts are significantly different from short GRBs but share many properties with long bursts, probably pointing to a common progenitor type. However, we find that intermediate bursts are significantly dimmer and have on average lower redshifts.
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