Chebyshev-derived spindown parameters for gravitational wave signals from pulsars
Keyword(s):
The master equation described by Badri Krishnan et al. (Phys Rev. D, 70, 082001 (2004)) for the time-frequency pattern using the F-statistic is studied in the context of Chebyshev-polynomial modified spindown parameters for the case of gravitational wave 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.PACS Nos.: 04.30.Tv, 95.85.sz, 02.30.Gp, 02.40.Re
1990 ◽
Vol 80
(6B)
◽
pp. 2143-2160
2013 ◽
Vol 24
(04)
◽
pp. 1350017
◽
Keyword(s):
2007 ◽
Vol 07
(02)
◽
pp. 215-227
◽
2020 ◽