\begin{table}%t1
\caption{Photometric parameters for the MS~0451 sample.}
\label{tabrun2}
\small%\centerline
 {
\begin{tabular}{lllccccccc}
\hline\hline
ID &    RA      &       Dec &     $z$    &    $V$  &    $R$  &    $I$  & $M_B$   &  A  & C \\
$(1)$ & $(2)$ &$(3)$ & $(4)$ &$(5)$ & $(6)$ &$(7)$ & $(8)$ &$(9)$ & $(10)$ \\
\hline
C1 & 04:54:2.2   & --02:57:10 & 0.5421 & 21.94 & 20.85 & 19.95 & --21.06  & 0.25219    &     0.32179 \\
C2 & 04:54:17.2  & --03:01:56 & 0.5486 & 22.02 & 21.00 & 20.07 & --20.91  & 0.15682    &     0.34844 \\
C3 & 04:54:18.6  & --03:01:03 & 0.5465 & 22.16 & 21.20 & 20.49 & --20.68  & 0.07922    &     0.27806 \\
C4 & 04:54:17.6  & --02:59:23 & 0.5324 & 22.34 & 21.41 & 20.72 & --20.37  & 0.36244    &     0.33291 \\
C5 & 04:54:1.5   & --02:59:24 & 0.5312 & 22.42 & 21.01 & 19.81 & --20.82  & 0.15670    &     0.52285 \\
C6 & 04:54:1.3   & --02:59:22 & 0.5305 & 21.83 & 21.15 & 20.59 & --20.59  & 0.32947    &     0.40650 \\
C7 & 04:54:5.0   & --02:59:40 & 0.5277 & 19.75 & 19.23 & 18.86 & --22.45  & 0.32994    &     0.20636 \\
C8 & 04:54:4.4   & --03:00:14 & 0.5325 & 20.80 & 20.10 & 19.46 & --21.68  & 0.27380    &     0.27789 \\
C9 & 04:54:15.0  & --03:00:22 & 0.5246 & 20.56 & 19.89 & 19.46 & --21.76  & 0.33459    &     0.26970 \\
C10 & 04:54:17.7 & --03:02:29 & 0.5312 & 21.92 & 21.61 & 21.21 & --20.05  & 0.19672    &     0.21096 \\
C11 & 04:54:10.3 & --03:00:46 & --      &   --    &   --    &   --    &   --	&   --	     &  	--  \\
F1 & 04:54:2.7  & --02:58:41 & 0.9009 & 23.27 & 22.75 & 21.46 & --20.97  & 0.18516    &	  0.18578 \\
F2 & 04:54:3.8  & --02:59:19 & 0.5795 & 20.88 & 20.11 & 19.42 & --21.96  & 0.27311    &	  0.22909 \\
F3 & 04:54:14.9 & --02:58:17 & 0.5667 & 21.88 & 21.24 & 20.64 & --20.66  & 0.33834    &	  0.20427 \\
F4 & 04:54:7.8  & --03:00:33 & 0.1867 & 20.54 & 20.37 & 20.00 & --18.78  & 0.17365    &	  0.32308 \\
F5 & 04:54:10.0 & --03:00:28 & 0.1573 & 19.05 & 18.72 & 18.26 & --19.95  & 0.19844    &	  0.30783 \\
F6 & 04:54:18.9 & --03:00:05 & 0.0982 & 19.23 & 18.93 & 18.55 & --18.56  & 0.14823    &	  0.27114 \\
F7 & 04:54:2.3  & --02:58:10 & 0.9125 & 22.22 & 21.91 & 20.73 & --21.64  & 0.42715  &	 0.16334 \\
F8 & 04:54:10.4 & --03:00:47 & 0.4443 & -- & -- & -- &    --     &   --	    &	       --  \\
F9 & 04:54:10.2 & --03:01:57 & 0.3259 & 20.83 & 20.03 & 19.08 & --20.15  & 0.29565    &     0.53731 \\
F10 & 04:54:0.5  & --02:58:15 & 0.4947 & 22.47 & 21.86 & 21.38 & --19.67  & 0.20119    &     0.23420 \\
F11 & 04:54:20.6 & --03:00:16 & --      & 21.25 & 20.67 & 20.04 & --	& 0.18512   &	 0.27344 \\
\hline
\end{tabular}}
\medskip
Column (1): object ID; Cols.~(2,~3): RA and Dec (J2000);
Col.~(4): object redshift; Cols.~(5$-$7): $V$, $R$, $I$~extinction corrected total magnitudes from
the FORS2/VLT images;
Col.~(8): rest frame Johnson-$B$ magnitudes $k$-corrected with {\tt kcorrect} \citep{BR07};
Col.~(9): asymmetry index;
Col.~(10): concentration index. \\
For F11, the redshift is uncertain as explained in
Sect.~2.3.  Redshift of galaxy~F7 and~C11 are taken from \citet{M08}.  Galaxy~C11
and~F8 are so close together on the FORS images that their magnitudes could not be
measured separately. 
\end{table}