  We extend the treatment of the problem of the gravitational waves produced by
a particle of negligible mass orbiting a Kerr black hole using black hole
perturbation theory in the time domain, to elliptic and inclined orbits. We
model the particle by smearing the singularities in the source term using
narrow Gaussian distributions. We compare results (energy and angular momentum
fluxes) for such orbits with those computed using the frequency domain
formalism.
