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Table 9:

List of the photometric and morphologic quantities of measurable arcs and arc candidates, except for RBS-0864 (see Kausch et al. 2007) and RBS1316 (RXJ1347-1145, see Bradac et al. 2005). See text for more details.
Cluster Arc I R V B $\langle (V-R)\rangle$ (V-R) l/w Distance to Distance to Mass
    [mag] [mag] [mag] [mag] clusterg arcs   cc [ $^{\prime \prime }$] cc [ h-170 kpc] [ $\times 10^{14}~{M}_\odot$]
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 -
  B2a - $23.61\pm0.07$ $24.32\pm0.08$ - 0.72 $0.70\pm0.15$ 2.0 $\sim$50 $\sim$150 -
  B3a - - - - - - - $\sim$20 $\sim$60 -
RBS-0312 GGL1b - - - - - - - $\sim$2.4 $\sim$11 $\rm0.0104^{+0.004}_{-0.002}$ )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 $\rm0.52^{+0.35}_{-0.04}$
  A2 - - - - - - - $\sim$12 $\sim$30 $\rm0.123^{+0.08}_{-0.01}$)f
  B3 - $21.38\pm0.01$ $22.79\pm0.09$ - 0.59 $0.58\pm0.20$ 2.8 $\sim$37 $\sim$100 -
RBS-0653 GA1d - - - - - - - $\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 $\rm0.25^{+0.10}_{-0.04}$
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 $\rm0.41^{+0.25}_{-0.04}$
  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 $\rm0.45^{+0.28}_{-0.45}$
RBS-1748 B1e - $25.09\pm0.05$ $25.27\pm0.14$ - 0.57 $0.18\pm0.18$ 2.25 $\sim$31 $\sim$115 -
  B2 - $24.78\pm0.04$ $25.11\pm0.14$ - 0.57 $0.33\pm0.18$ 1.95 $\sim$35 $\sim$130 -

Notes.  (a) merging with another object; (b) galaxy-galaxy lensing candidate; (c) mass of the single galaxy with GGL1; (d) GA = giant arc; (e) measured on the HST frame; (f) mass of the BCG; (g) averaged colour of the five brightest cluster galaxies.


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