  Two classes of gamma-ray bursts have been identified in the BATSE catalogs
characterized by durations shorter and longer than about 2 seconds. There are,
however, some indications for the existence of a third class. Swift satellite
detectors have different spectral sensitivity than pre-Swift ones for gamma-ray
bursts. Therefore, it is worth to reanalyze the durations and their
distribution. We analyze, the maximum likelihood estimation, the bursts
duration distribution, published in The First BAT Catalog, whether it contains
two, three or more groups. The three log-normal fit is significantly (99.54%
probability) better than the two for the duration distribution. Monte-Carlo
simulations also confirm this probability (99.2%). Similarly, in previous
results we found that the fourth component is not needed. The relative
frequencies of the distribution of the groups are 7% short 35% intermediate and
58% long. Although the relative frequencies of the groups are different than in
the BATSE GRB sample, the difference in the instrument spectral sensitivities
can explain this bias on a natural way. This means theoretical models may be
needed to explain three different type of gamma-ray bursts.
