Fig. 7.
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Best-fit model SEDs to the 15 spectra of NGC 5548 (dotted grey lines). The solid black line shows the average of the 15 SEDs. The solid red line corresponds to the best-fit model to the time-averaged SED. Blue circles indicate the average flux of the 15 segments in the UV bands. The orange shaded areas highlight the energy ranges used to fit the time-averaged SED.
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