Chebyshev Derived Spindown Parameters for Gravita- Tional Wave Signals from Pulsars
نویسندگان
چکیده
The master equation described by Badri Krishnan et al. [1] for the time-frequency pattern using the F-statistic is studied in context of the Chebyshev polynomial modified spindown parameters for the case of gravitational wave (GW) pulsar signals. The Chebyshev polynomial method enables an analytic and numeric evaluation of the Fourier transform (FT) for both the non-demodulated and F-statistic demodulated FT (DeFT). NOTE: FIX NUMBERING ISSUES IN THE EQN ARRAYS
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تاریخ انتشار 2007