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Gravitational-wave signals from compact binary coalescences are most efficiently identified through matched filter searches, which match the data against a pre-generated bank of gravitational-wave templates.
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A. Buonanno, Y.-b. Chen, Y. Pan, and M. Vallisneri, “A Quasi-physical family of gravity-wave templates for precessing binaries of spinning compact objects. 2. Application to double-spin precessing binaries,” Phys. Rev. D
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PhD thesis, Bologna U., 2009
D. Fazi, Development of a Physical-Template Search for Gravitational Waves from Spinning Compact-Object Binaries with LIGO · 2009
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