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It was recently shown that the $T_{90}-H_{32}$ distributions of gamma-raybursts from CGRO/BATSE and Fermi/GBM are well described by a mixture of onlytwo skewed components, making the presumed third, intermediate classunnecesary. The Swift/BAT, Konus-Wind, RHESSI and Suzaku/WAM data sets arefound to be consistent with a two-class description as well.

Analysis of the duration$-$hardness ratio plane of gamma-ray bursts with skewed distributions