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We study whether binary black hole template banks can be used to search for the gravitational waves emitted by general binary coalescences.
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K. G. Arun, B. R. Iyer, B. S. Sathyaprakash, and P. A. Sundararajan, “Parameter Estimation of Inspiralling Compact Binaries using 3.5 Post-Newtonian Gravitational Wave Phasing: The Non-spinning Case,” Phys. Rev
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T. Damour, B. R. Iyer, and B. Sathyaprakash, “A Comparison of Search Templates for Gravitational Waves from Binary Inspiral,” Phys. Rev. D
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