| Abstract | 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 16J<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 six individual galaxies. Partly based on observations at European Southern Observatory (ESO) at the ESO Schmidt Telescope and the 1.52 m telescope under the ESO-ON agreement; Observatório do Pico dos Dias, operated by the Laboratório Nacional de Astrofísica (LNA); and Complejo Astronomico El Leoncito (CASLEO), operated under agreement between the Consejo Nacional de Investigaciones Científicas de la República Argentina and the National Universities of La Plata, Córdoba, and San Juan. |
