SEDs and best-fit DUSTY models for the dusty AGB stars. Solid blue line: input spectra; solid red line: total DUSTY model; dotted cyan line: attenuated input spectral component; dashed green line: dust scattered component; dot-dashed orange line: dust thermal component. Photometric fluxes are indicated as filled circles (in a few cases the variability-induced uncertainties are larger than the average value), photometric data not included in the analysis as empty circles, and upper limits as empty triangles. Solid grey lines are GAIA, IRAS, and ISO spectra; shadowed areas indicate 10% uncertainties.