In this section, we study the detection of a deterministic gravitational-wave signal of the general
form given by Eq. (32
) and the estimation of its parameters
using the maximum-likelihood (ML)
principle. We assume that the noise
in the detector is a zero-mean, Gaussian, and stationary random
process. The data
in the detector, in the case when the gravitational-wave signal
is present, is
. The parameters
of the signal (32
) split into extrinsic (or amplitude)
parameters
and intrinsic ones
.
http://www.livingreviews.org/lrr-2012-4 |
Living Rev. Relativity 15, (2012), 4
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