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 (21
) 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 [34]. This property is independent of the probability distribution of the noise.
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