  We introduce a set of four new publicly available N-body simulations, the
most recent additions to the Texas P^3M Database. Our models probe the less
studied parameter space region of moderate volume (100/h Mpc box) combined with
fine mass resolution (~10^12 M_Sol, roughly comparable to a L_* galaxy), making
these simulations especially suitable for study of major large-scale structure
features such as voids, and for comparison with the largest three-dimensional
redshift surveys currently available. Our cosmological models (LCDM, TOCDM,
OCDM, TCDM) are all COBE-normalized, and when possible (LCDM and TOCDM) also
cluster-normalized, based on the X-ray cluster M--T relation. The COBE- and
cluster-normalized LCDM model reiterates the attractiveness of this currently
favored model which does not require the introduction of tilt in order to fit
the constraints imposed by observations of other cosmological parameters.
