\begin{table}%t1
\caption{Overview of model parameters. From left to right, the columns 
indicate: planet mass in \mearth, value of the adiabatic exponent ($\Gamma=1$
means a locally isothermal equation of state), viscosity parameter~$\alpha$,
radiation flag, accretion flag and the number of refinement levels. When
$n_{\rm lev}$~levels of refinement are used, the local resolution within
a distance of $2H$ from the planet is a factor~$2^{n_{\rm lev}}$ higher
than the base resolution of $\Delta r=0.0082~r_{\rm p}$. For the local 
models, the indicated resolution is valid for the whole computational domain.}
\label{table:1}
%\centering
\small
\begin{tabular}{c c c c c c c c}
\hline\hline
$M_{\rm p}$ (\mearth) & $\Gamma$ & $\alpha$ & FLD & Acc & $n_{\rm lev}$
& $\mathcal{S}$ & Comments \\
\hline
0.6 & 1 & 0.004 & n & y & 5 & 0 &\\
5   & 1 & 0.004 & n & y & 4 & 0 &\\
5   & 1 & 0.004 & n & y & 3 & 0 &\\
5   & 1 & 0.004 & n & y & 2 & 0 &\\
40  & 1 & 0.004 & n & y & 3 & 0 &\\
320 & 1 & 0.004 & n & y & 2 & 0 &\\
\hline
5   & 1.005 & 0 & n & y & 4 & --0.9925 &\\ 
5   & 1.01  & 0 & n & y & 4 & --0.9850 &\\ 
5   & 1.005 & 0 & n & y & 3 & --0.9925 &\\ 
5   & 1.01  & 0 & n & y & 3 & --0.9850 &\\ 
\hline
0.6 & 1.4   & 0 & y & n & 5 & --0.4 &\\
0.6 & 1.4   & 0 & y & y & 5 & --0.4 &\\
0.6 & 1.4   & 0 & y & n & 4 & --0.4 &\\
0.6 & 1.4   & 0 & y & y & 4 & --0.4 &\\
5   & 1.4   & 0 & y & n & 4 & --0.4 &\\
5   & 1.4   & 0 & y & y & 4 & --0.4 &\\
5   & 1.4   & 0 & y & n & 3 & --0.4 &\\
5   & 1.4   & 0 & y & y & 3 & --0.4 &\\
5   & 1.4   & 0 & y & n & 2 & --0.4 &\\
5   & 1.4   & 0 & y & y & 2 & --0.4 &\\
5   & 1.4   & 0 & y & n & 4 & --0.4 & 10 times lower density\\
5   & 1.4   & 0 & y & n & 4 & --0.4 & 100 times lower density\\
\hline
5   & 1.4   & 0 & n & n & 4 & --0.4 &local model\\
5   & 1     & 0 & n & n & 4 & 0 & local model\\
5   & 1.4   & 0 & n & n & 4 & --0.2 & local model\\ 
5   & 1.4   & 0 & n & n & 4 & 0.2 & local model\\ 
5   & 1.4   & 0 & n & n & 4 & 0.4 & local model\\ 
\hline
\end{tabular}
\end{table}