Fig. 8.
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IDV wavelet analysis performed on the dereddened, host-galaxy-subtracted R-band flux light curves of 3C 371 for sectors 18 (left) and 22 (right). Top: R-band light curves. Bottom: time-period power spectra. White contours represent variability signatures with a significance > 3σ (> 99.73% confidence level). Gray grids represent the cone of influence regions affected by edge effects.
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