Fig. B.1.
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MBSEDs (in the observer’s frame) for the ten QSOs with the highest colour excess E(g − z). The flux is in units of erg s−1 cm−2 Å−1. The black squares with error bars are the fluxes from photometric data; the SDSS spectra are plotted in green (both corrected for Galactic foreground extinction). The template spectrum for bright QSOs of type 1 from Polletta et al. (2007) is shown in blue.
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