  This study developed an automated identification procedure for compact clouds
with broad velocity widths in the spectral line data cubes of highly crowded
regions. The procedure was applied to the CO J=3-2 line data, obtained using
the James Clerk Maxwell Telescope, to identify 184 high velocity dispersion
compact clouds (HVCCs), which is a category of peculiar molecular clouds found
in the central molecular zone of our galaxy. A list of HVCCs in the area
-1.4{\deg}<l<+2.0{\deg}, -0.25{\deg}<b<+0.25{\deg} was presented with their
physical parameters, CO J=3-2/J=1-0 intensity ratios, and morphological
classifications. Consequently, the list provides several intriguing sources
that may have been driven by encounters with point-like massive objects, local
energetic events, or cloud-to-cloud collisions.
