Gravitational waves from inspiraling compact binaries: Accuracy of the post-Newtonian waveforms
arXiv:gr-qc/9801038
Abstract
The accuracy of the post-Newtonian waveforms, both in standard and Pade form, is determined by computing their matched-filtering overlap integral with a reference waveform obtained from black-hole perturbation theory.
3 pages, ReVTeX, to appear in the Proceedings of the Second Gravitational Wave Data Analysis Workshop, held in Orsay, France