\begin{table}%t3
\caption{Gravitational wave frequencies (in Hz) computed from  the calculated data for GNH3, APR and BPAL12~EOSs:  the $f_{\rm npm}$ denotes the frequency at which the non-point-mass effects start to be important, $f_{\rm 20}, f_{\rm 25}$ and~$f_{\rm 40}$ are the so-called break-frequencies (see text), whereas~$f_{\rm end}$ is the  GW~frequency on the final orbit.}
\label{ftable}
%\centering
\par
\begin{tabular}{cccccc}
\hline\hline
\multicolumn{1}{c}{EOS} &
\multicolumn{1}{c}{$f_{\rm npm}$} &
\multicolumn{1}{c}{$f_{\rm 20}$} &
\multicolumn{1}{c}{$f_{\rm 25}$}&
\multicolumn{1}{c}{$f_{\rm 40}$} &
\multicolumn{1}{c}{$f_{\rm end}$} \\
\hline
GNH3 &500&567&657&792&806  \\
APR &700&615&762&1025& 1132  \\
BPAL12 &1050&615&785&1160&1270  \\
\hline
\end{tabular}
\end{table}