# Reliability of complete gravitational waveform models for compact binary coalescences

@article{Ohme2011ReliabilityOC, title={Reliability of complete gravitational waveform models for compact binary coalescences}, author={Frank Ohme and Mark D. Hannam and Sascha Husa}, journal={Physical Review D}, year={2011}, volume={84}, pages={064029} }

Accurate knowledge of the gravitational-wave (GW) signal from inspiraling compact binaries is
essential to detect these signatures in the data from GW interferometers. With recent advances in post-
Newtonian (PN) theory and numerical relativity (NR) it has become possible to construct inspiral-mergerringdown
waveforms by combining both descriptions into one complete hybrid signal. While addressing
the reliability of such waveforms in different points of the physical parameter space… Expand

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