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Fig. 7

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35–100 keV versus 14–24 keV variability estimator for the AGN in our sample. The dashed line indicates where objects with the same variability in the two bands would lie. Even though the variations in the two bands are well correlated, the variations in the lower-energy band are larger than those at higher energies for the majority of the radio quiet objects. Some of the most extreme outliers are labeled.

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