centra

Accuracy of the post-Newtonian approximation. II. Optimal asymptotic expansion of the energy flux for quasicircular, extreme mass-ratio inspirals into a Kerr black hole

Compact stars in alternative theories of gravity: Einstein-Dilaton-Gauss- Bonnet gravity

Comparing numerical and analytical calculations of post-innermost stable circular orbit ringdown amplitudes

Constraining properties of the black hole population using LISA

Erratum: Accuracy of the post-Newtonian approximation: Optimal asymptotic expansion for quasicircular, extreme-mass ratio inspirals (Physical Review D - Particles, Fields, Gravitation and Cosmology (2008) 77 (124006))