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Fig. 6.

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Wavelet spectrograms for GRB 230307A for all three instruments. In all three, we find significant power at the lowest frequencies, as well as power at 1.2 Hz. In white contours, we overplot the 99.99% percentiles. In the Fermi/GBM data, we mark the segment flagged by the Fermi team for potential data issues as the shaded region.

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