  The RIT numerical relativity group is releasing a public catalog of
black-hole-binary waveforms. The initial release of the catalog consists of 126
recent simulations that include precessing and non precessing systems with mass
ratios $q=m_1/m_2$ in the range $1/6\leq q\leq1$. The catalog contains
information about the initial data of the simulation, the waveforms
extrapolated to infinity, as well as information about the peak luminosity and
final remnant black hole properties. These waveforms can be used to
independently interpret gravitational wave signals from laser interferometric
detectors and
