Observed spectral energy distributions (red data points) overlaid with the best-fit spectral models (solid black lines) for the 231 successfully fitted ATLAS^3D galaxies. AKARI data points are shown as stars; other data points are shown as filled circles. Dotted orange, green, red, and blue lines indicate the best-fit stellar, PAH, warm, and cold dust component, respectively. The name of the galaxy is indicated in the top left corner of each panel, in blue for CO-detected galaxies and red for non-CO-detected galaxies. Galaxies with no AKARI FIR (65, 90 or 140μm) detection are marked with an asterisk. The full figure is available in Appendix B.