\begin{table}%T2
\caption{Parameters of the \LkCa\ disk derived from the model fits. \label{tab:fit-lkca15} }
\small%\centerline
{
\begin{tabular}{lcc}
\hline \hline
\multicolumn{3}{c}{Temperature from CO isotopologues} \\
 $T_{100}$ (K) & \multicolumn{2}{c}{$22 \pm 1$} \\
 $q$ &  \multicolumn{2}{c}{$0.37 \pm 0.02 $} \\
 \hline
  \multicolumn{3}{c}{Derived parameters from 2.8 and 1.4~mm dust emission} \\
 $R_{\rm int}$ (AU) & $46 \pm 3$ & [5]$^a$ \\
 $R_{\rm out}$ (AU) & $177 \pm 12$ & $135 \pm 3$ \\
 $\Sigma_{100}$ (g~cm$^{-2}$) & $3.1\pm 0.4$ & $4.1 \pm 0.6$ \\
 $p$ & $1.7 \pm 0.3$ & $-0.5 \pm 0.2$  \\
 $\beta$ & $1.2 \pm 0.1$ & $1.1 \pm 0.1$  \\
 $M_{\rm disk}$ ($\msun$) & 0.029 & 0.025 \\
 \hline
\end{tabular}}
\smallskip
{The error bars are the $1\sigma$ formal errors (effective noise, see Sect.~2) from the fit. Two solutions are
presented: one with a free inner radius, and one with a fixed inner radius of 5~AU. The dust emission is too
optically thin to allow us an independent fit of the temperature, which is adopted from the CO analysis
presented in \citet{Pietu_etal2006}. $^a$ Square brackets indicate fixed parameters.}
\end{table}