\begin{table}%t8
\caption {\label{tbl:rejfrac_maglim.tab}Total fraction of galaxies rejected as cluster members as a function of
the $I$~magnitude (Cols.~3 to~6 for $I\ge 22$, 23, 24 and 24.5~\mbox{respectively}). }
%\centerline
 {\begin{tabular}{lccccc}
\hline \hline
Cluster & $z_{\rm cl}$ & $f_{22}$ & $f_{23}$ & $f_{24}$ & $f_{24.5}$ \\
\hline
Cl1018.5-1211 & 0.4734 & 0.68 & 0.77 & 0.85 & 0.88 \\
Cl1037.5-1243a & 0.4252 & 0.50 & 0.58 & 0.71 & 0.77 \\
Cl1040.4-1156 & 0.7043 & 0.68 & 0.73 & 0.83 & 0.86 \\
Cl1054.2-1146 & 0.6972 & 0.56 & 0.67 & 0.78 & 0.83 \\
Cl1054.4-1245 & 0.7498 & 0.58 & 0.60 & 0.69 & 0.75 \\
Cl1059.1-1253 & 0.4564 & 0.68 & 0.76 & 0.84 & 0.87 \\
Cl1103.4-1245b & 0.7031 & 0.72 & 0.77 & 0.83 & 0.86 \\
Cl1119.2-1129 & 0.5500 & 0.69 & 0.75 & 0.81 & 0.83 \\
Cl1122.5-1136 & 0.6397 & 0.61 & 0.66 & 0.79 & 0.84 \\
Cl1138.1-1133 & 0.4796 & 0.53 & 0.62 & 0.74 & 0.79 \\
Cl1202.4-1224 & 0.4240 & 0.80 & 0.86 & 0.91 & 0.93 \\
Cl1216.4-1201 & 0.7943 & 0.62 & 0.66 & 0.74 & 0.78 \\
Cl1227.5-1138 & 0.6357 & 0.58 & 0.64 & 0.73 & 0.77 \\
Cl1232.3-1250 & 0.5414 & 0.67 & 0.73 & 0.82 & 0.85 \\
Cl1238.3-1144 & 0.4602 & 0.65 & 0.73 & 0.81 & 0.83 \\
Cl1301.4-1139 & 0.4828 & 0.71 & 0.79 & 0.87 & 0.90 \\
Cl1353.0-1137 & 0.5882 & 0.77 & 0.84 & 0.89 & 0.91 \\
Cl1354.1-1231 & 0.7620 & 0.64 & 0.66 & 0.75 & 0.78 \\
Cl1411.0-1148 & 0.5195 & 0.81 & 0.84 & 0.90 & 0.92 \\
Cl1420.2-1236 & 0.4962 & 0.82 & 0.87 & 0.91 & 0.93 \\
\hline
\end{tabular}}
\par
\smallskip
Notes: only galaxies with NIR data were used in this calculation,
except for Cl1119-1129 and Cl1238-1144. For these two
clusters, all galaxies were used because no NIR data exists.
\end{table}