Modelling Gravitational Waves from Inspiralling Compact Binaries

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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

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