\begin{table}%t4
\caption{\label{offsets}Conunterparts of the radio detections.} 
\small%\centerline
{
\begin{tabular}{lcccccc}
\hline\hline
\noalign{\smallskip}
Radio  & Optical/IR  & $d_{\rm obs}$  & $r_{\rm src}$  & $P_{\rm assoc.}$\\ 
source & source      & (arcsecs)  & (arcsecs)  & ($\%$)          \\
\noalign{\smallskip}
\hline 		
\noalign{\smallskip}        
E1     & B1$^\ast$   & 0.38       &  0.6       & 67.8          \\
\noalign{\smallskip}
\hline 		
\noalign{\smallskip}	       	
CR1    & ARC 1.1     & 1.12       &  0.15      & $<$1         \\
       & ARC 2.1     & 1.40       &  0.25      & $<$1        \\
       & ARC 3.1     & 1.60       &  0.20      & $<$1         \\
\noalign{\smallskip}
\hline 		
\noalign{\smallskip}		          
CR2    & G2          & 1.39       &  0.70       &  $<$1          \\
       & C2$^\ast$   & 1.82       &  0.60       &  $<$1        \\
       & ARC 1.2     & 1.92       &  0.15       &  $<$1      \\
\noalign{\smallskip}
\hline 		
\noalign{\smallskip}		          
E2     & B2$^\ast$   & 0.26       &  0.60       & 79.29        \\
       & G10         & 0.74       &  0.23       & $< $1     \\
\noalign{\smallskip}
\hline 		
\noalign{\smallskip}		            
E3     & 4.3$^\ast$   & 0.77       &  0.60       & 20.7         \\
       & 5.3$^\ast$   & 1.22       &  0.30       & $<$1        \\ 
       & G23         & 1.54       &  0.35       & $< $1      \\ 
\noalign{\smallskip}
\hline 	
\noalign{\smallskip}		            
RJ     & G8          & 1.91       &  0.30       & $<$1     \\
       & G11         & 2.40       &  0.26       & $<$1     \\
       & G14         & 1.39       &  0.60       & $<$1     \\
\hline				             
\end{tabular}}
\smallskip
The columns
show: possible counterparts of the radio detections (Optical/IR
source), mesured offset between the radio source and the optical/IR
source ($d_{\rm obs}$), radius of the optical/IR source ($r_{\rm
src}$) and probability that the centroid of the radio source lies
inside the area of the optical/IR source ($P_{\rm assoc.}$). The
coordinates of the counterpart sources can be found in Tables~\ref{tab_catalog} and~\ref{tab_constrains}. Sources which positions
were taken from the $K'$~band image are indicated with an asterisk
(otherwise we used the HST coordinates). The positions of the radio
sources used to calculate~$d_{\rm obs}$ correspond to the values
derived with {\sc  maxfit} in the aligned radio map. 
\end{table}