Modelling Gravitational Waves from Inspiralling Compact Binaries
arXiv:gr-qc/9801014
Abstract
Gravitational waves from inspiralling compact binaries can be reliably extracted from a noisy detector output only if the template used in the detection is a faithful representation of the true signal. In this article we suggest a new approach to constructing faithful signal models.
Needs sprocl.sty which is bundled together with the tex file. To appear in the proceedings "Second Edoardo Amaldi Conference on Gravitational Waves", CERN, 1 - 4 July 1997