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Fig. 19.

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Preliminary RL relation for the UV Fe II pseudo-continuum based on the two time-lag measurements for NGC 5548 (Maoz et al. 1993) and CTS C30.10 (this work). We derive two relations based on the two Fe II time delays for CTS C30.10: 180.3 days and 270.0 days. The longer time delay of 270.0 days is more consistent with the RL relation derived by Bentz et al. (2013) when renormalized to the 3000 Å monochromatic luminosity. The shaded regions depict 1σ confidence intervals of individual RL relations.

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