Fit of two sources with a large luminosity ratio that cannot be explained with the KERRBB radiation pattern. The SDSS spectrum (black line) continuum is described with KERRBB (dashed red line, with a shaded blue area representing a confidence interval given by the uncertainty on the spectrum peak; see Sect. 4.1) while the torus emission is constrained with the four WISE data points (red dots) and two black bodies (shaded red area with a dashed blue line contour) plotted along with the corresponding temperatures. The thick blue line is the overall model (disk + torus). On each plot, we report the isotropic disk and torus luminosities (in erg s⁻¹) and the luminosity ratio R along with its uncertainty (see Sect. 5.3). Some archival photometric data (2MASS, NED, GALEX – gray dots) are added to both plots. The yellow shaded area is the luminosity range in which ν_pL_νp lies, obtained by taking into account different uncertainties (Sect. 5.3).