Model results using the parameters from Reidemeister et al. (2011) in comparison with the observed disk profiles (upper panel) and the SED (bottom panel). In the disk profile plot, the observed profiles are symbols with gray areas marking the upper and lower boundaries of uncertainty due to flux calibration and PSF subtraction. Red circles are the FORCAST 35 μm data, and blue squares are the MIPS 24 μm data. Model profiles are shown in solid lines with green color for 35 μm and orange for 24 μm. In the bottom SED plot, the various symbols are the excess photometry measurements for the whole system, and the green dots with error bars are the excess from the IRS and MIPS-SED spectra. The gray area around the IRS excess spectrum represents the uncertainty associated with the stellar photospheric extrapolation and subtraction. The model SED is composed of two parts: the red (the dragged-in small grains inside 10 au) and blue solid lines (the rest of the dragged-in grains and the dust in the cold planetesimal belt (P.B.)) with the sum shown as the black dash line (replicated from the bottom panel of Figure 8 in Reidemeister et al. 2011).