Fig. 4 Power and wavelet spectra of benthic δ18O.

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Fig. 4 Power and wavelet spectra of benthic δ18O. Power and wavelet spectra of benthic δ18O. (A) Power spectra of modeled δ18O (blue) compared to power spectra of the δ18O stack of (3) (black) for different time intervals, as indicated above the panels. Wavelet spectra of (B) the benthic δ18O stack of (3) and (C) modeled δ18O. Black contours indicate the 5% significance level against red noise. The horizontal white lines represent the orbital periods of precession (∼23 ka), obliquity (∼41 ka), and eccentricity (∼100 ka). The model spectra are derived from the average δ18O computed over all ensemble members resulting from the time-splitting technique. M. Willeit et al. Sci Adv 2019;5:eaav7337 Copyright © 2019 The Authors, some rights reserved; exclusive licensee American Association for the Advancement of Science. No claim to original U.S. Government Works. Distributed under a Creative Commons Attribution License 4.0 (CC BY).