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Fig. 7.

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IDV wavelet analysis performed on the dereddened, host-galaxy-subtracted R-band flux light curve of 3C 371. Top: R-band light curve. Middle: time-period power spectrum (left) and time-folded power spectrum (right). White contours in the left panel and the dashed line in the right panel represent variability signatures with a significance > 3σ (> 99.73% confidence level). Bottom: averaged variance between 4 min and 1 day. The horizontal dashed line represents the 3σ (99.73%) confidence level.

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