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The phase parameters of matched-filtering searches for continuous gravitational-wave signals are sky position, frequency and frequency time-derivatives.
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The effects of the neutron star’s proper motion in this context are discussed in [ 8 , 18 ] . Assuming an extreme case where the star moves with respect to the SSB at 10 3 km / s 10^{3}\,{\rm km/s} and its distance to the detector to be at 40 pc 40\,{\rm pc} , over 120 days of observation, fitting factors (fraction of signal-to-noise ratio when using a filter not perfectly matching to a signal) greater than 99% are obtained. In addition, in this paper observation times of order a few days, much less than 120 days, are considered and therefore the proper-motion effects are neglected
Cited in the paper.
The maximum Doppler frequency shift due to the Earth motion is given approximately by the maximum Earth’s orbital velocity v orb / c ≈ 10 − 4 v_{\rm orb}/c\approx 10^{-4}
Cited in the paper.
The LSC Algorithm Library Applications, available at http://www.lsc-group.phys.uwm.edu/daswg/
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H. J. Pletsch, in preparation
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B. Abbott et al. (The LIGO Scientific Collaboration), Phys. Rev. D 77
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B. Abbott et al. (The LIGO Scientific Collaboration), Phys. Rev. D 79
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