Spectral energy distribution fit (blue line) for two beamed AGN sources. The black dots indicate archival data, the error bars are shown in gray, the red pointers represent the upper limits, and the purple crosses depict the mean flux in a 0.1 width logarithmic bin of frequency. The model considers a phenomenological description of the jet emission for blazar-like sources with the optional addition of an emitting thin accretion disk (cyan dashed line) and an obscuring torus (green dashed line).