\begin{table}%t1
\caption{\label{tab_maxfit_R0.6}Information about the identifyed radio sources in
 the core of MS0451.} 
 \small %\centerline
{
\begin{tabular}{lcccccccccc}
\hline\hline 
\noalign{\smallskip}
Name & RA ($+4^{\rm h}$ $54^{\rm m}$) & Dec ($- 3^{\circ}$)         & $S_{\rm Pk}$      & $S_{2\sigma}$ & $S_{\rm CC}$ & $S_{\rm resid}$ & $\frac{S_{\rm CC} - S_{2\sigma}}{S_{2\sigma}}$   & $\frac{S_{\rm CC} - S_{\rm Gauss}}{S_{\rm Gauss}}$  & {\it SNR} \\ 
                    & J2000 (s)            & J2000 ($\arcmin$,$\arcsec$)& ($\rm \mu Jy~beam^{-1}$) & ($\mu$Jy)  & ($\mu$Jy)   & ($\mu$Jy)  &  ($\%$)                              &   ($\%$)                        &     &      \\
\noalign{\smallskip}
\hline 
\noalign{\smallskip}
E1        & $12.78 \pm 0.01$ & $00:43.8 \pm 0.2$ & $66\pm10$ & $42.5 \pm12$ & 61.6  & -1.4  & 45  &  17  & 6.4    \\
CR1       & $12.88 \pm 0.01$ & $00:53.5 \pm 0.2$ & $47\pm10$ & $36.6 \pm12$ & 47.2  & 2.9   & 29  & $-16$  & 4.6   \\
CR2       & $12.86 \pm 0.01$ & $00:59.3 \pm 0.2$ & $47\pm10$ & $43.8 \pm12$ & 60.1  & -0.1 & 37  & $-21$  & 4.6   \\
E2        & $12.66 \pm 0.01$ & $01:01.2 \pm 0.2$ & $51\pm10$ & $43.2 \pm12$ & 52.0  & 5.1   & 20  & $-15$  & 5.0   \\
RJ bright & $12.54 \pm 0.01$ & $01:17.2 \pm 0.1$ & $92\pm10$ & $121.2\pm17$ & 135.9 & --    & 12  & $-17$  & 8.9   \\
RJ        & $12.54 \pm 0.01$ & $01:17.2 \pm 0.1$ & $92\pm10$ & $168.0\pm22$ & 195.3 & 10.5  & 16  & --   & 8.9   \\ 
E3        & $10.97 \pm 0.01$ & $01:24.8 \pm 0.2$ & $54\pm10$ & $63.3 \pm15$ & 66.8  & 6.5  & 5   & $-28$  & 5.2    \\		  
\noalign{\smallskip}                                                                         
\hline		  
\noalign{\smallskip}		  
%Fb    &          & $          $ &          &  &  &   &   & 3.97     \\
Fd    & $15.162  \pm 0.003  $ & $01:10.83 \pm 0.05$ & $199 \pm10$  & $1180.9\pm42 $ & 1260  & 29.5   & 7  & --  & 19.2      \\
Fe    & $09.2733 \pm 0.0007 $ & $00:50.90 \pm 0.01$ & $1068\pm10$  & $1769.2\pm34 $ & 1870  & 16.3   & 6  & --  & 103.3     \\
\hline
\end{tabular}}
\smallskip
The columns show: position (RA, Dec), peak flux
 density ($S_{\rm Pk}$), total flux density inside the 2$\sigma$~contour ($S_{\rm 2\sigma}$), total flux density obtained by adding
 the flux from all the clean components used to model the source ($S_{\rm CC}$), total flux density inside the 2$\sigma$ contour in
 the residual map ($S_{\rm resid}$), comparison between the total flux
 derived from the CC~model and the $2~\sigma$ contours $\left(
 \frac{S_{\rm CC} - S_{2\sigma}}{S_{2\sigma}} \right)$, comparison
 between the total flux derived from the CC~model and the Gaussian fit
 $\left( \frac{S_{\rm CC} - S_{\rm Gauss}}{S_{\rm Gauss}} \right)$ and
 signal-to-noise ratio (SNR). The quoted errors in RA and DEC
 correspond to the expected positional uncertainty of a point-like
 source in the map ($\emph{FWHM} / 2 \times \emph{SNR}$, were
 \emph{FWHM} is the full with half maximum of the clean beam), while
 the error in the flux peak is estimated to be the same as the rms
 noise of the map. The error in the $2\sigma$ flux was calculated as
 ${\rm rms} \times \sqrt{N}$, where  rms  is the rms noise of the map,
 and \emph{N} is the number of beams within the area delimited by the
 $2\sigma$ contour of the source. The raw ``RJ bright'' lists the
 fluxes for RJ estimated withouth taking into account the $4\sigma$
 west extension. Note that the positions listed here were derived
 before aligning the radio map respect to the HST image.
\end{table}