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Accuracy of the post-Newtonian approximation for extreme mass ratio inspirals from a black-hole perturbation approach

Gravitational waves from a particle in circular orbits around a rotating black hole to the 11th post-Newtonian order

Comparison of post-Newtonian templates for extreme mass ratio inspirals

Erratum: Post-Newtonian factorized multipolar waveforms for spinning, nonprecessing black-hole binaries (Physical Review D - Particles, Fields, Gravitation and Cosmology (2011) 83 (064003))

Evolution of the Carter constant for resonant inspirals into a Kerr black hole: I. the scalar case