\begin{table}%T2
\caption{\label{tab:Tab2}VLBI detection rates for the 447 weak extragalactic radio sources observed during EC025A and EC025B. In this study, \textit{detection} means that at this frequency the ${\it SNR} \geq 7$, for at least one scan on one baseline.}
\small%\centering
\par
\begin{tabular}{lcccc}        
\hline\hline 
\noalign{\smallskip}
                & \textbf{Sources}  & $\vec X$\textbf{-band}    & $\vec S$\textbf{-band}    & $\vec S$ \textbf{and} $\vec X$  \\
                & \textbf{observed} & \textbf{detection} & \textbf{detection} & \textbf{detection}\\
%\noalign{\smallskip}               
\hline                       
\noalign{\smallskip}  
\textbf{EC025A} & 218               &   216 sources      &   211 sources      &  211 sources      \\  
                &                   &         99\%       &         96\%       &       96\%        \\ 
%\noalign{\smallskip}               
%\hline                       
\noalign{\smallskip}  
\textbf{EC025B} & 229               &   216 sources      &   188 sources      &  187 sources      \\ 
                &                   &         94\%       &         82\%       &       82\%        \\ 
%\noalign{\smallskip}               
%\hline                       
\noalign{\smallskip}    
\textbf{Overall}& 447               &   432 sources      &   399 sources      &  398 sources      \\
                &                   &         97\%       &         89\%       &       89\%        \\ 
\hline                        
\end{tabular}
\end{table}