\begin{table}%t1
%\centering
\par
\caption{\label{tab1} Parameters chosen in the different
simulations and their results. These parameters are the dimensioning of the grid ($n_r, n_\vartheta,n_\varphi$),
the kind of spacing (lc = logarithmically centered around the planet), 
the thermodynamics (iso = locally isothermal, rad = ideal gas plus radiation transport, rad+ = ideal gas,
radiation transport and conservation of total energy for gas accreted onto planet), the gravitational smoothing radius ($q_{\rm g}$ = fraction of the Hill radius over that smoothing is applied), the accretion radius ($q_{\rm acc}$ = fraction of the Roche lobe (respectively Hill radius) that mass is taken out of), the type of the initial model (G: starting with an
existing gap), and the total number of orbits calculated ($t_{\rm int}$). The results we give are the accretion rate onto the Planet ($\dot M$) in units of Jupiter masses per orbit, the mass contained in the Roche lobe ($M_{\rm Roche}$), the maximum density and temperature in the Roche lobe ($\rho_{\rm max}, T_{\rm max}$) and the migration time-scale that we determined ($\tau_{\rm mig}$).}
\begin{tabular}{l l l l l r l l l r l}
\hline
\hline
{Name}  & {Grid}                    &{EOS}& {$q_{\rm g}$; $q_{\rm a}$}&{ini}&{$t_{\rm max}$}&{$\dot M$}&{$M_{\rm Roche}$}&{$\rho_{\rm max}$}&{$T_{\rm max}$}&{$\tau_{\rm mig}$} \\
\hline
%\startdata
{CI}    &$100\times20\times 1  $    & iso  & 0.5   ; 0.5 &         & $300$ & --                  &     --             & $2.0\times10^{-14}$ &$130$& -- \\  %(prev. modCI:   ant3   )
{CDI}   &$100\times20\times 200$    & iso  & 0.5   ; 0.5 & G       & $184$ & $1.5\times10^{-4}$ & $2.2\times10^{-5}$& $3.0\times10^{-13}$ &$130$& $8.9\times10^{4}$  \\   
{CD4I}  &$100\times24\times 200$ lc & iso  & 0.2   ; 0.2 & G       & $81$  & $1.2\times10^{-4}$ & $3.2\times10^{-5}$& $0.9\times10^{-11}$ &$130$& $1.0\times10^{5}$          \\    
{CD}    &$100\times20\times 200$    & rad  & 0.5   ; 0.5 & G       & $142$ & $6.0\times10^{-4}$ & $6.5\times10^{-5}$& $1.0\times10^{-12}$ &$150$& $7.8\times10^{4}$          \\     
{CDS}   &$100\times20\times 200$    & rad  & 0.2   ; 0.2 & G       & $141$ & $3.0\times10^{-4}$ & $1.3\times10^{-4}$& $2.0\times10^{-12}$ &$200$& $8.2\times10^{4}$  \\      
{CD4}   &$100\times24\times 200$ lc & rad  & 0.2   ; 0.2 & G       & $75$  & $4.0\times10^{-4}$ & $8.0\times10^{-5}$& $2.0\times10^{-11}$ &$480$& $8.0\times10^{4}$  \\  
{CDNI}  &$100\times20\times 200$    & iso  & 0.5   ; 0   & G       & $98$  &    --               & $3.3\times10^{-4}$& $5.0\times10^{-11}$ &$130$& $8.3\times10^{4}$  \\  
{CDN}   &$100\times20\times 200$    & rad  & 0.5   ; 0   & G       & $44$  &    --               & $7.5\times10^{-3}$& $6.0\times10^{-11}$ &$310$& $8.9\times10^{4}$  \\  
{CDN4}  &$100\times24\times 200$ lc & rad  & 0.2   ; 0   & G       & $122$ &    --               & $3.6\times10^{-4}$& $4.0\times10^{-10}$ &$520$& $1.2\times10^{5}$  \\   
{DN}    &$100\times20\times 200$    & rad  & 0.5   ; 0   &         & $121$ &    --               & $1.3\times10^{-3}$& $7.0\times10^{-11}$ &$600$& $6.6\times10^{4}$  \\  
{DN4}   &$100\times24\times 200$ lc & rad  & 0.2   ; 0   &         & $55$  &    --               & $1.7\times10^{-2}$& $2.0\times10^{-9} $ &$1150$&    \\   
{DR}    &$100\times25\times 200$    & rad+ & 0.2   ; 0.2 &         & $121$ & $6.5\times10^{-4}$ & $5.5\times10^{-4}$& $2.0\times10^{-11}$ &$800$& $1.0\times10^{5} $  \\  
{DR4}   &$100\times25\times 200$ lc & rad+ & 0.1   ; 0.1 &         & $141$  & $3.5\times10^{-4}$ & $4.5\times10^{-4}$& $4.5\times10^{-10}$ &$1500$& $1.2\times10^{5} $    \\   
\hline
\end{tabular}
\end{table}