Time series analysis by projection .1. Statistical properties of Fourier analysis

被引:74
作者
Foster, G
机构
[1] Amer. Assoc. Variable Star Observers, Cambridge, MA 02138
关键词
D O I
10.1086/117805
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Most time series analysis methods are equivalent to treating the data as a vector in function space, then projecting the data vector onto a subspace of low dimension. By casting various Fourier methods in terms of projection, we can make their behaviors transparent and adapt them to time series with irregular time spacing. Exact statistics are derived for the discrete Fourier transform, the Lomb-Scargle modified periodogram [Lomb, APSS, 39, 447 (1976); Scargle, APJ, 263, 835 (1982)], and the date-compensated discrete Fourier transform [Ferraz-Mello; AJ, 86, 619 (1981)]. Fourier methods have an extra complication, that they are not merely projections but parametric projections. As a consequence, the standard statistical evaluation of Fourier analysis (and most period-search methods) is incomplete. (C) 1996 American Astronomical Society.
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页码:541 / 554
页数:14
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