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We investigate methods to estimate the parameters of the gravitational-wavesignal from a spinning neutron star using Fourier transformed segments of thestrain response from an interferometric detector. Estimating the parametersfrom the power, we find generalizations of the PowerFlux method. Usingsimulated elliptically polarized signals injected into Gaussian noise, we applythe generalized methods to estimate the squared amplitudes of the plus andcross polarizations (and, in the most general case, the polarization angle),and test the relative detection efficiencies of the various methods.

Using generalized PowerFlux methods to estimate the parameters of periodic gravitational waves