SED of the best fits of the cold disk and warm belt models. The green curve corresponds to the warm and cold dust emissions added to the Next Gen stellar atmosphere spectrum (gray). IRS spectrum is in red. We also show separately the best fit of the warm belt emission (r_w = 0.2 AU and m_w = 2.8 × 10^-6 M_$) (yellow) and the best fit of the cold disk emission (parameters of the combined fit are in Table 3) (blue). Insets and photometric data points are the same as in the legend of Fig. 6.