We first present the false alarm and detection probabilities when the intrinsic parameters of the signal are known. In this case the -statistic is a quadratic form of the random variables that are correlations of the data. As we assume that the noise in the data is Gaussian and the correlations are linear functions of the data, is a quadratic form of the Gaussian random variables. Consequently the -statistic has a distribution related to the distribution. One can show (see Section III B in ) that for the signal given by Eq. (30), has a distribution with degrees of freedom when the signal is absent and noncentral distribution with degrees of freedom and non-centrality parameter equal to the square of the signal-to-noise ratio when the signal is present.
As a result the pdfs and of the -statistic, when the intrinsic parameters are known and when respectively the signal is absent or present in the data, are given byfalse alarm probability is the probability that exceeds a certain threshold when there is no signal. In our case we have probability of detection is the probability that exceeds the threshold when a signal is present and the signal-to-noise ratio is equal to : [132, 58], . We see that when the noise in the detector is Gaussian and the intrinsic parameters are known, the probability of detection of the signal depends on a single quantity: the optimal signal-to-noise ratio .
Next we return to the case in which the intrinsic parameters are not known. Then the statistic given by Eq. (62) is a certain multiparameter random process called the random field (see monographs [5, 6] for a comprehensive discussion of random fields). If the vector has one component the random field is simply a random process. For random fields we define the autocovariance function just in the same way as we define such a function for a random process:
One can estimate the false alarm probability in the following way . The autocovariance function tends to zero as the displacement increases (it is maximal for ). Thus we can divide the parameter space into elementary cells such that in each cell the autocovariance function is appreciably different from zero. The realizations of the random field within a cell will be correlated (dependent), whereas realizations of the random field within each cell and outside of the cell are almost uncorrelated (independent). Thus, the number of cells covering the parameter space gives an estimate of the number of independent realizations of the random field.
We choose the elementary cell with its origin at the point to be a compact region with boundary defined by the requirement that the autocovariance between the origin and any point at the cell’s boundary equals half of its maximum value, i.e., . Thus, the elementary cell is defined by the inequality
To estimate the number of cells we perform the Taylor expansion of the autocovariance function up to the second-order terms:, Appendix B) that the matrix is precisely equal to the reduced Fisher matrix given by Eq. (81).
If the components of the matrix are constant (i.e., they are independent of the values of the intrinsic parameters of the signal), the above equation defines a hyperellipsoid in -dimensional ( is the number of the intrinsic parameters) Euclidean space . The -dimensional Euclidean volume of the elementary cell given by Eq. (95) equalslinear function of the intrinsic parameters .
To estimate the number of cells in the case when the components of the matrix are not constant, i.e., when they depend on the values of the intrinsic parameters , one replaces Eq. (97) by, where an analogous integral formula was proposed for the number of templates needed to perform a search for gravitational-wave signals from coalescing binaries.
The concept of number of cells was introduced in  and it is a generalization of the idea of an effective number of samples introduced in  for the case of a coalescing binary signal.
We approximate the pdf of the -statistic in each cell by the pdf of the -statistic when the parameters are known [it is given by Eq. (84)]. The values of the -statistic in each cell can be considered as independent random variables. The probability that does not exceed the threshold in a given cell is , where is given by Eq. (86). Consequently the probability that does not exceed the threshold in all the cells is . Thus, the probability that exceeds in one or more cells is given by.
It was shown (see ) that for any finite and , Eq. (99) provides an upper bound for the false alarm probability. Also in  a tighter upper bound for the false alarm probability was derived by modifying a formula obtained by Mohanty . The formula amounts essentially to introducing a suitable coefficient multiplying the number of cells.
When the signal is present in the data a precise calculation of the pdf of the -statistic is very difficult because the presence of the signal makes the data’s random process non-stationary. As a first approximation we can estimate the probability of detection of the signal when the intrinsic parameters are unknown by the probability of detection when these parameters are known [it is given by Eq. (87)]. This approximation assumes that when the signal is present the true values of the intrinsic parameters fall within the cell where the -statistic has a maximum. This approximation will be the better the higher the signal-to-noise ratio is.
Living Rev. Relativity 15, (2012), 4
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