Examples of eight SED fits. The overall fit (including reddening) is shown as the black line. In the case of type-1 objects, the dashed magenta line shows the unreddened quasar template. In the case of type-2 objects, or objects not classified as AGN in their optical spectra, the red line is the best-fit stellar population, and the dashed cyan line the mid-infrared AGN template fit. The dashed vertical line is at a rest wavelength of 5 μm, indicating the wavelength at which we measure the AGN flux density.