\begin{table}%t2
\caption{\label{table:IsoForSigma15}Isolated formation of Jupiter and Saturn for a disk with surfaces densities of solids and gas ${\propto}a^{-3/2}$.}
\par
%\centering
\par
\begin{tabular}{lllllllll}
\hline \hline \noalign{\smallskip}
MM & & Jupiter & & & & Saturn & & \\
SN & & & & & &  & & \\ 
& $\Sigma_{\rm s}$ 
 & $\rho_{\rm g}$ 
 & $M_{\rm c}$
 & $t_{\rm f}$ 
 & $\Sigma_{\rm s}$ 
 & $\rho_{\rm g}$ 
 & $M_{\rm c}$  
 & $t_{\rm f}$ \\
\hline
                 4 & 10.12 & 2.54 & 21.31 & 5.34 &  ---  & ---  &  ---  &  --- \\  
  5 & 12.65 & 3.17 & 26.61 & 2.86 &  ---  & ---  &  ---  &  --- \\  
  6 & 15.18 & 3.81 & 31.35 & 1.76 &  6.14 & 0.73 & 17.07 & 9.62 \\
  7 & 17.71 & 4.45 & 36.32 & 1.09 &  7.17 & 0.85 & 20.83 & 4.89 \\
  8 & 20.24 & 5.08 & 41.48 & 0.62 &  8.19 & 0.97 & 23.76 & 2.85 \\
  9 & 22.77 & 5.72 & 45.39 & 0.33 &  9.22 & 1.09 & 26.38 & 1.75 \\
 10 & 25.30 & 6.35 & 46.09 & 0.16 & 10.24 & 1.21 & 28.72 & 1.08 \\
\hline 
\end{tabular}
\tablefoot {\tablefoottext{*}{$\Sigma_{\rm s}~[{\rm g~cm}^{-2}]$ and $\rho_{\rm g}~[10^{-11}~{\rm g~cm}^{-3}]$ are the initial surface density of solids and the initial volumetric density of gas at the disk mid-plane at the position of Jupiter and Saturn, respectively. $M_{\rm c}~[M_{\oplus}]$~is the final core mass and $t_{\rm f}~[{\rm Myr}]$ is the formation time.}}
\end{table}