Broadband SED of J1430 (red data points), covering ten orders of magnitude in wavelength. The leftmost points are the 2–7 keV and 0.5–2 keV fluxes from Chandra, respectively, as fitted by the best fit MYTorus model. The range of data points from ∼0.1−100 μ m have been fit with SED3FIT 20 times and the median fit is shown in black, with the colored strips labeling the 68% margins of the distributions for all the components. The host galaxy component of the fit is shown in orange, the AGN torus contribution is shown as green dashes and the star formation component is in cyan. The SED is typical of an obscured AGN, with the optical light dominated by the host galaxy. Based on the fit of this portion of the SED, we can infer both a reliable measure of the stellar mass of the host and the bolometric luminosity of the AGN. The rightmost data points show, in red, the core radio SED, while the gray points display the lobes emission.