\begin{table}%t9 \par \caption {\label{tab:arclist1}List of the photometric and morphologic quantities of measurable arcs and arc candidates, except for RBS-0864 \citep[see][]{kausch07a} and RBS1316 \citep[RXJ1347-1145, see][]{bradac05a}. See text for more details. } %\centerline {\begin{tabular}{c c c c c c c c c c c c } \hline\hline Cluster & Arc & $I$ & $R$ & $V$ & $B$ & $\langle (V-R)\rangle$ & $(V-R)$ & $l/w$ & Distance to & Distance to & Mass\\ & & [mag] & [mag] & [mag] & [mag] & cluster$^g$ & arcs & & cc [\arcsec] & cc [$h^{-1}_{70}$~kpc] & [$\times 10^{14}~{M}_\odot$]\\ \hline RBS-0172 & B1 & -- & $23.28\pm0.02$ & $24.16\pm0.07$ & -- & 0.72 & $0.88\pm0.09$ & 1.5 & $\sim$$29$ & $\sim$$120$ & -- \\ RBS-0238 & B1 & -- & $22.42\pm0.04$ & $23.31\pm0.05$ & -- & 0.72 & $0.89\pm0.10$ & 2.5 & $\sim$$20$ & $\sim$$60$ & -- \\ & B2$^a$& -- & $23.61\pm0.07$ & $24.32\pm0.08$ & -- & 0.72 & $0.70\pm0.15$ & 2.0 & $\sim$$50$ & $\sim$$150$ & -- \\ & B3$^a$& -- & -- & -- & -- & -- & -- & -- & $\sim$20 & $\sim$$60$ & --\\ RBS-0312 & GGL1$^b$ & -- & -- & -- & -- & -- & -- & -- & $\sim$2.4 & $\sim$11 & $\rm 0.0104^{+0.004}_{-0.002}$ $)^c$ \\ RBS-0325 & A1 & -- & $21.02\pm0.01$ & $21.48\pm0.02$ & $21.79\pm0.03$ & 0.84 & $0.47\pm0.02$ & 1.7 & $\sim$$50$ &$\sim$$210$ & $\rm 4.04^{+1.73}_{-0.64}$\\ & B2 & -- & $22.58\pm0.01$ & $23.38\pm0.07$ & $24.09\pm0.23$ & 0.84 & $1.80\pm0.08$ & 1.7 & $\sim$$47$ &$\sim$$200$ & --\\ & A3 & -- & $22.89\pm0.03$ & $24.29\pm0.12$ & $24.60\pm0.30$ & 0.84 & $1.40\pm0.15$ & 2.6 & $\sim$$30$ &$\sim$$130$ & $\rm 1.48^{+0.63}_{-0.23}$\\ & B4 & -- & -- & -- & -- & -- & -- & -- & $\sim$$38$ &$\sim$$162$ & $\rm 2.38^{+1.01}_{-0.37}$\\ RBS-0436 & B1 & -- & $23.04\pm0.05$ & $23.47\pm0.01$ & -- & 0.56 & $0.42\pm0.06$ & 2.7 & $\sim$$41$ &$\sim$$130$ & -- \\ RBS-0651 & A1 & -- & $21.11\pm0.01$ & $22.31\pm0.05$ & -- & 0.59 & $1.20\pm0.05$ & 2.5 & $\sim$$25$ & $\sim$$67$ & $\rm 0.52^{+0.35}_{-0.04}$ \\ & A2 & -- & -- & -- & -- & -- & -- & -- & $\sim$$12$ & $\sim$$30$ & $\rm 0.123^{+0.08}_{-0.01}$)$^f$\\ & B3 & -- & $21.38\pm0.01$ & $22.79\pm0.09$ & -- & 0.59 & $0.58\pm0.20$ & 2.8 & $\sim$$37$ & $\sim$$100$ & --\\ RBS-0653 & GA1$^d$ & -- & -- & -- & -- & -- & -- & -- & $\sim$$20$ & $\sim87$ & $\rm 6.67^{+2.80}_{-1.07}$ \\ & GA2 & -- & -- & -- & -- & -- & -- & -- & $\sim$$11$ & $\sim$$47$ & $\rm 2.02^{+0.85}_{-0.32}$\\ & GA3 & -- & -- & -- & -- & -- & -- & -- & $\sim$$19$ & $\sim$$82$ & $\rm 6.02^{+2.53}_{-0.97}$\\ & A3 & $18.12\pm0.01$ & $19.23\pm0.01$ & $20.28\pm0.01$ & $21.38\pm0.09$ & 1.93 & $1.05\pm0.08$ & 2.1 & $\sim$$12$ & $\sim$$52$ & $\rm 0.25^{+0.10}_{-0.04}$ \\ RBS-1015 & B1 & -- & $23.79\pm0.04$ & $24.62\pm0.02$ & -- & 0.66 & $0.83\pm0.06$ & 1.9 & $\sim$$38$ & $\sim$$145$ & -- \\ RBS-1029 & B1 & -- & $22.36\pm0.03$ & $23.12\pm0.03$ & -- & 0.59 & $0.76\pm0.06$ & 1.9 & $\sim$$37$ & $\sim$$105$ & -- \\ RBS-1460 & B1 & -- & $23.39\pm0.07$ & $24.06\pm0.07$ & -- & 0.65 & $0.67\pm0.15$ & 2.2 & $\sim$$42$ & $\sim$$148$ & -- \\ RBS-1712 & A1 & $22.66\pm0.05$ & -- & $23.29\pm0.02$ & -- & -- & -- & 2.6 & $\sim$$20$ &$\sim$$63$ & $\rm 0.41^{+0.25}_{-0.04}$ \\ & A2 & $23.34\pm0.05$ & $24.17\pm0.13$ & $23.70\pm0.02$ & -- & 0.64 & $-0.47\pm0.15$ & 1.9 & $\sim$$21$ & $\sim$$66$ & $\rm 0.45^{+0.28}_{-0.45}$ \\ RBS-1748 & B1$^e$ & -- & $25.09\pm0.05$ & $25.27\pm0.14$ & -- & 0.57 & $0.18\pm0.18$ & 2.2$^5$ & $\sim$$31$ & $\sim$115 & --\\ & B2 & -- & $24.78\pm0.04$ & $25.11\pm0.14$ & -- & 0.57 & $0.33\pm0.18$ & 1.9$^5$ & $\sim$$35$ & $\sim$$130$ & --\\ \hline \end{tabular}} \tablefoot { \tablefoottext{a}{merging with another object;} \tablefoottext{b}{galaxy-galaxy lensing candidate;} \tablefoottext{c}{mass of the single galaxy with GGL1;} \tablefoottext{d}{GA~=~giant arc;} \tablefoottext{e}{measured on the HST frame;} \tablefoottext{f}{mass of the BCG;} \tablefoottext{g}{averaged colour of the five brightest cluster galaxies.}} \end{table}