A method for the estimation of the significance of cross-correlations in unevenly sampled red-noise time series
W. Max-Moerbeck, J.L. Richards, T. Hovatta, V. Pavlidou, T.J. Pearson,, A.C.S. Readhead

TL;DR
This paper introduces an improved Monte Carlo method for assessing the significance of cross-correlations in unevenly sampled red-noise time series, addressing challenges like red-noise leakage and model estimation.
Contribution
It presents novel normalization, bootstrap significance estimation, and error analysis techniques for cross-correlation in unevenly sampled data with red noise.
Findings
High cross-correlations can occur in unrelated light curves with steep power spectra.
Interpolation and Hanning window reduce red-noise leakage effects.
The method reliably estimates significance and errors in power spectral density indices.
Abstract
We present a practical implementation of a Monte Carlo method to estimate the significance of cross-correlations in unevenly sampled time series of data, whose statistical properties are modeled with a simple power-law power spectral density. This implementation builds on published methods, we introduce a number of improvements in the normalization of the cross-correlation function estimate and a bootstrap method for estimating the significance of the cross-correlations. A closely related matter is the estimation of a model for the light curves, which is critical for the significance estimates. We present a graphical and quantitative demonstration that uses simulations to show how common it is to get high cross-correlations for unrelated light curves with steep power spectral densities. This demonstration highlights the dangers of interpreting them as signs of a physical connection. We…
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