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Gravitational waves from inspiralling binaries are expected to be detected using a data analysis technique known as matched filtering. This technique is applicable whenever the form of the signal is known accurately. Though we know the form of the signal precisely, we will not know a priori its parameters. Hence it is essential to filter the raw output through a host of search templates each corresponding to different values of the parameters. The number of search templates needed in detectingdoi:10.1103/physrevd.50.r7111 pmid:10017762 fatcat:uuwfgsihirbk5jm4abj3rqpupm