\begin{table}%t1
\caption{Cosmological simulations of structure formation analysed in
  this study.}\label{tabSimulations}
%\centering
\small
\begin{tabular}{cp{6.5cm}ccccc}
\hline
\hline
Name & Physics & $L$  & Resolution & $m_{\rm DM}$
 & $m_{\rm gas}$    & $\epsilon_{\rm grav}$  \\ 
 &  & [$h^{-1}~{\rm Mpc}$] &  & [$h^{-1}~{M}_\odot$] &  [$h^{-1}~{M}_\odot$]  &  [$h^{-1}~{\rm kpc}$] \\
\hline
%&&&&&& \\[-8pt]
S1 & non-radiative, no star formation (SF) & 
$100$ & $2\times 256^3$   & $4.30\times 10^9$ & $6.62\times 10^8$ &  $15.0$ \\
\hline
%&&&&&& \\[-8pt]
S2 & CR-injection at shocks with $\zeta_{\rm inj}=0.5$,
  $\alpha_{\rm inj}=2.5$, no
  star formation & $100$ & $2\times 256^3$   & $4.30\times 10^9$ & $6.62\times 10^8$ &  $15.0$ \\
\hline
%&&&&&& \\[-8pt]
S3 & Mach-number dependent CR injection at shocks, no
  star formation & $100$ & $2\times 256^3$   & $4.30\times 10^9$ & $6.62\times 10^8$ &  $15.0$ \\
\hline
%&&&&&& \\[-8pt]
D1 & radiative cooling, star formation (SF), no cosmic rays & 
$10$ & $2\times 256^3$   & $4.30\times 10^6$ & $6.62\times 10^5$ &  $1.3$ \\
\hline
%&&&&&& \\[-8pt]
D2 & radiative cooling, SF, CRs from supernovae (SNe) & $10$ & $2\times 256^3$   & $4.30\times 10^6$ & $6.62\times 10^5$ &  $1.3$ \\
\hline
%&&&&&& \\[-8pt]
D3 & radiative cooling, SF, CRs from SNe and
shocks (according to Mach-number)   & $10$ & $2\times 256^3$   & $4.30\times 10^6$ & $6.62\times 10^5$ &  $1.3$ \\
\hline
\end{tabular}
\end{table}