  An extreme mass ratio inspiral takes place when a compact stellar object is
inspiraling into a supermassive black hole due to gravitational radiation
reaction. Gravitational waves (GWs) from this system can be calculated using
the Teukolsky equation (TE). In our case, we compute the asymptotic GW fluxes
of a spinning body orbiting a Kerr black hole by solving numerically the TE
both in time and frequency domain. Our ultimate goal is to produce GW templates
for space-based detectors such as LISA.
