  We present spectroscopic and photometric data for 920 galaxies selected in 68
fields of the Aquarius Cluster Catalog. Typically the 15 brightest candidate
members with magnitudes in the range 16 < b_J < 21 were selected for
observations, and ~ 71% turn out to be cluster members. Using the new redshift
determinations we assign galaxies to groups and clusters, and by including data
from the literature we calculate systemic velocities and velocity dispersions
for 74 clusters, each with redshifts measured for at least 6 individual
galaxies.
