\begin{table}%t1
%\centering
\par
\caption {\label{tab:simus}Cosmological hydrodynamical simulations studied in this \mbox{paper}.}
{
\begin{tabular}{lcccc}\hline \hline
\noalign{\smallskip}
Name & F/NF  &  $N_{\rm p}$ & $M_{\rm dark}$ & $M_{\rm gas}  $  \\ 
     &       &              &$[10^6~ {M}_{\odot}~ h^{-1}]$ & $[10^6~ {M}_{\odot}~ h^{-1}]$ \\ \hline\\[-3.5mm]
S160 & F    & $2 \times160^3$  & $17.6$  &  $2.71$    \\ 
S230 & F   & $2 \times230^3$  & $5.93$  &  $0.91$    \\ 
S230NF & NF    & $2 \times230^3$  & $5.93$  &  $0.91$    \\ 
S320 & F   & $2 \times320^3$  & $2.20$  &  $0.34$    \\ 
\hline 
\end{tabular}
}
\tablefoot {Column~2: Model with/without SN feedback (F/NF). 
Column 3: Initial number of particles in the simulation. 
Column 4: Mass of dark matter particles. 
Column 5: Initial mass of gas particles.}
\end{table}