Fig. 3.

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Flare peak and post-flare SEDs and the best-fitting AGNSED model. In the right panel, we present the (observed and absorbed/reddened) data and the best-fitting models. In the left column, we have corrected both data and models for Galactic absorption and reddening. In both panels, black and purple data points denote, respectively, flaring and post-flaring state data. XMM-Newton pn data have been rebinned by a factor of 4 for plotting purposes only. In both panels, red and blue lines denote, respectively, the best-fitting models to the flaring and post-flaring states. The dashed lines denote the best-fitting AGNSED components, the grey dashed line represents the host galaxy template, and the solid lines represent the total models.
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