Spectral energy distribution fits for eight central stars. Top row: Two examples of SED fits for stars that do not show an IR excess. Remaining spectra: Multicomponent SED fits for the stars in our sample that show a near- and/or far-infrared excess. Black dots correspond to observed photometry; the blue and purple shaded areas correspond to the flux contribution of the CS and a cool blackbody, respectively; and the dark purple line is the (combined) best fit to the observation.