The duration distribution of Swift Gamma-Ray Bursts
  Decades ago two classes of gamma-ray bursts were identified and delineated as
having durations shorter and longer than about 2 s. Subsequently indications
also supported the existence of a third class. Using maximum likelihood
estimation we analyze the duration distribution of 888 Swift BAT bursts
observed before October 2015. Fitting three log-normal functions to the
duration distribution of the bursts provides a better fit than two log-normal
distributions, with 99.9999% significance. Similarly to earlier results, we
found that a fourth component is not needed. The relative frequencies of the
distribution of the groups are 8% for short, 35% for intermediate and 57% for
long bursts which correspond to our previous results. We analyse the redshift
distribution for the 269 GRBs of the 888 GRBs with known redshift. We find no
evidence for the previously suggested difference between the long and
intermediate GRBs' redshift distribution. The observed redshift distribution of
the 20 short GRBs differs with high significance from the distributions of the
other groups.
