  We evolve a binary black hole system bearing a mass ratio of $q=m_1/m_2=2/3$
and individual spins of $S^z_1/m_1^2=0.95$ and $S^z_2/m_2^2=-0.95$ in a
configuration where the large black hole has its spin antialigned with the
orbital angular momentum, $L^z$, and the small black hole has its spin aligned
with $L^z$. This configuration was chosen to measure the maximum recoil of the
remnant black hole for nonprecessing binaries. We find that the remnant black
hole recoils at 500km/s, the largest recorded value from numerical simulations
for aligned spin configurations. The remnant mass, spin, and gravitational
waveform peak luminosity and frequency also provide a valuable point in
parameter space for source modeling.
