Spectral energy distributions (SEDs) of planet hosts and planet host candidates. The dotted line represents the stellar photosphere model for the spectral type of the star scaled to the dereddened J-band flux. Open and solid dots are observed and dereddened fluxes, respectively. Symbols in gray are WISE fluxes. The two longest wavelength flux upper limits are the Herschel/PACS observations. For comparison, the SEDs of η Crv (Duchêne et al. 2014) and β Pic (Vandenbussche et al. 2010) have been normalized to the dereddened J-band flux and added to each plot denoted by dashed and dot-dashed lines, respectively.