Let
be the gravitational-wave signal and let
be the detector noise. For convenience we assume that the signal
is a continuous function of time
and that the noise
is a continuous random process. Results for the discrete time
data that we have in practice can then be obtained by a suitable
sampling of the continuous-in-time expressions. Assuming that the
noise is
additive
the data
can be written as
From the expression (19
) we see immediately that the likelihood ratio test consists of
correlating the data
with the signal
that is present in the noise and comparing the correlation to a
threshold. Such a correlation is called the
matched filter
. The matched filter is a linear operation on the data.
An important quantity is the optimal
signal-to-noise ratio
defined by
An interesting property of the matched filter is that it maximizes the signal-to-noise ratio over all linear filters [28] . This property is independent of the probability distribution of the noise.
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