\begin{table}%t3
\caption{\label{table_fitparam}Adopted and fitted parameters for our model of AB~Aur disk.}
\par
%\centerline
{\small
\begin{tabular}{lcc}
\hline\hline
Stellar fixed parameters & & Ref.\\
\hline
Stellar Luminosity ($L_{*}$ )& $ 47 \Lsun$ & 8 \\
Effective Temperature ($T_{\rm eff}$) & 9333 K &  8 \\
\hline
Adopted fixed parameters & & Ref.\\
\hline
Distance $D$ & 144~pc&  \\
% & & \\
Inner Radius ($R_{\rm in}$) & 0.30~AU & 5, 6\\
Outer Radius ($R_{\rm out}$) & 200~AU & 3\\
Inclination	 ($i$) & $33\deg$ & 2, 3, 6, 7\\
%& & \\
Dust Mass ($M_{\rm d}$ )& $5\times 10^{-5}\Msun$ &  1, 2, 3, 4 \\
Dust grain Density & 2 g~cm$^{-3}$ &  \\
Dust Composition & 62.5\% amorp. silicates & \\
 & 37.5\% graphite & \\
 Grains size & [0.005--0.250]\micron & \\
Sublimation Temperature ($T_{\rm sub}$) & 1500 K & \\
\hline
Fitted parameters & Value~$[\pm 3\sigma]$ & $\chi^2_{\rm r~tot}$\\
\hline
\qquad With {ISO spectrum} & \\
$\beta$ & $1.27~[\pm 0.025]$  & 2.93\\
$h_{100}$~[AU] & $8.0~[\pm 0.5]$& \\
\qquad With {MIDI spectrum}  &\\
$\beta$ & $1.27~[\pm 0.025]$  & 3.74\\
$h_{100}$~[AU] & $8.0~[\pm 0.5]$& \\
\hline
\end{tabular}}
\par
\medskip
Ref.: 1) \citet{man97}; 2) \citet{sem05}; 3) \citet{pie05}; 4) \citet{cor05}; 5) \citet{mil01}; 6)~\citet{eis04}; 7) \citet{pan05}; 8) \citet{her04}.
\end{table}