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Fig. 6.

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Averaged flare profiles of IRAS 13224–3809 with the corresponding ACFs. Left panel: Same as the upper right panel of Fig. 4, but the IRAS 13224–3809 flares are calculated from low- (red line), low-medium (black line), and high- (blue line) flux subsamples of the IRAS 13224–3809 light curve. Right panel: Mean ACFs of the same light-curve subsamples of IRAS 13224–3809.

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