Fig. 1.
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Examples of the observed SED along with the best-fit SED from CIGALE for one NLS1 galaxy (left panel) and one BLS1 galaxy (right panel). The open and filled symbols correspond to the observed and modelled flux densities. The goodness of the fit, represented by the reduced χ2, is given at the top of each plot. The residuals of the fit are given at the bottom of each panel.
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