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Table 8:

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 respectively).
Cluster $z_{\rm cl}$ f22 f23 f24 f24.5
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

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.

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