\begin{table}%t1
\caption{\label{frequencies}$\nu_0$ is the spin frequency of the targeted MSPs at the
time of the AURIGA run, whereas $\nu_{\rm gw} {\rm [Hz]}$ is the
frequency of the GW signal we searched for. }
%\centerline
{
\begin{tabular}{ccc}
\hline\hline
Name & $\nu_0$ [Hz] & $\nu_{\rm gw}$ [Hz] \\
\hline 
PSR J0024$-$7204J & 476.0468584406(...) & 952.0937168812(...) \\
PSR J0218+4232 &  430.4610663457(...) & 860.9221326914(...) \\
PSR J1939+2134 &  641.9282611068(...) & 855.9043481424(...) \\
\hline
\end{tabular}}
\smallskip
\par
Notice that, for the third
source, we are looking for the {\it r}-mode emission channel.
\end{table}