Table 1
Systems of multiple images employed in the model-based lens reconstructions.
| Image | RA [deg] | DEC [deg] | z | zm |
|---|---|---|---|---|
| 1.1 | 6.65528 | 17.15463 | 1.675 | |
| 1.2 | 6.65689 | 17.15678 | 1.675 | |
| 1.3 | 6.65832 | 17.16154 | 1.675 | |
| 1.4 | 6.64303 | 17.16495 | 1.675 | |
| 1.5 | 6.64724 | 17.16173 | 1.675 | |
| 3.1 | 6.65358 | 17.15675 |  |
 |
| 3.2 | 6.64858 | 17.17178 | 2.48 ± 0.34 | |
| 3.3 | 6.64475 | 17.17017 |  |
|
| 3.4 | 6.63717 | 17.16294 |  |
|
| 4.1 | 6.64413 | 17.16169 |  |
1.96 ± 0.20 |
| 4.2 | 6.64479 | 17.16153 |  |
|
| 4.3 | 6.66138 | 17.16072 |  |
|
| 5.1 | 6.63692 | 17.16092 |  |
2.02 ± 0.20 |
| 5.2 | 6.65317 | 17.15886 |  |
|
| 8.1 | 6.65158 | 17.14886 | 4.09 ± 0.50 | 4.03 ± 0.50 |
| 8.2 | 6.64588 | 17.16744 |  |
|
| 10.1 | 6.65071 | 17.16175 | 0.75 ± 0.17 |  |
| 10.2 | 6.65046 | 17.16186 |  |
|
| 10.3 | 6.64021 | 17.16183 |  |
|
Notes. The coordinates for system 1 are determined by visual inspection; this system is the only one with a spectroscopic redshift, the properties of the remaining systems are determined as described in Zitrin et al. (2009) with a BPZ photometric redshift estimation according to Benítez (2000); Benítez et al. (2004); Coe et al. (2006). For comparison with Zitrin et al. (2009), we keep their nomenclature (except for system 1) and also list the redshifts zm determined by their model.
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