  The third release of the RIT public catalog of numerical relativity
black-hole-binary waveforms \url{http://ccrg.rit.edu/~RITCatalog} consists of
777 accurate simulations that include 300 precessing and 477 nonprecessing
binary systems with mass ratios $q=m_1/m_2$ in the range $1/15\leq q\leq1$ and
individual spins up to $s/m^2=0.95$. The catalog also provides initial
parameters of the binary, trajectory information, peak radiation, and final
remnant black hole properties. The waveforms are corrected for the center of
mass drifting and are extrapolated to future null infinity. We successfully
test this correction comparing with simulations of low radition content initial
data. As an initial application of this waveform catalog we reanalyze all the
peak radiation and remnant properties to find new, simple, correlations among
them for practical astrophysical usage.
