2016
DOI: 10.1201/b15154
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Time Series with Mixed Spectra

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Cited by 30 publications
(39 citation statements)
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“…Note that the classical Fisher's test [20] standardizes the periodogram ordinates by the estimated PSD of a white noise. Standardization (2) can be seen as a generalization of this approach (see [24] for a recent review). The estimate S E (ν) can be parametric or non-parametric.…”
Section: B Unknown Noise Statistics: Related Workmentioning
confidence: 99%
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“…Note that the classical Fisher's test [20] standardizes the periodogram ordinates by the estimated PSD of a white noise. Standardization (2) can be seen as a generalization of this approach (see [24] for a recent review). The estimate S E (ν) can be parametric or non-parametric.…”
Section: B Unknown Noise Statistics: Related Workmentioning
confidence: 99%
“…A further complication arises when multiple sinusoids are present under the alternative, as they perturb the estimation of the noise PSD [5], [27]. Standardized tests for this case can be found in [21], [22], [24], [27]- [29]. These tests are however non adaptive in the number of sinusoids (which must be set a priori) and designed for white noise.…”
Section: B Unknown Noise Statistics: Related Workmentioning
confidence: 99%
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“…As remarked after the proposition, the error rate becomes O(T −3/2 ) for g(T ) equal to or greater than O(T 1/6 ). In the closely related time series setting, the unwindowed periodogram achieves the same rate when g(T ) is greater than O(T 1/2 ) (Theorem 6.8b of [13]). We will therefore examine ν − ν λ ∞ as a function of T at the frequency resolutions corresponding to g(T ) ∈ {6, T 1/6 , T 1/2 }.…”
Section: 1mentioning
confidence: 95%
“…Even if some of these estimators are asymptotically unbiased, the unavoidable injection of estimation noise in the denominator of the standardized periodogram makes the statistical characterization of the test statistics difficult. One can resort to Monte Carlo or bootstrap simulations [17] to evaluate the thresholds empirically (see [18], Chap.7 for examples of gaps between theoretical and empirical thresholds), but this procedure may not be tractable for massive time series (large N ). In Astronomy, preprocessing stages aimed at "whitening" the noise (e.g.…”
Section: Introductionmentioning
confidence: 99%