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Table A.2

Multiple-image systems found after the FF observations.

ID RA Dec zspec zmodel (non-cored, cored, NFW) zphot

20.1 109.37420 37.7651450 3.4 ± 1.0, >2.6, uncons.
20.2 109.37340 37.7646610
21.1* 109.37241 37.746392 2.61 ± 0.16
21.2* 109.37673 37.752029 2.65 ± 0.12
22.1* 109.36773 37.755897 0.87 ± 0.11
22.2* 109.36769 37.755556 0.93 ± 0.05
23.1* 109.37958 37.762879
23.2* 109.37897 37.761983
24.1 109.392290 37.732946 2.7 ± 0.1, 2.5 ± 0.1, 2.5 ± 0.1
24.2 109.410560 37.748427
25.1 109.380290 37.744746 4.0 ± 0.1, 3.8 ± 0.1, 3.8 ± 0.2
25.2 109.379510 37.742762
25.3 109.402910 37.766411
27.1 109.397390 37.747883 1.6 ± 0.9, 3.0 ± 1.1, uncons. 2.95 ± 0.18
27.2 109.397560 37.747567 2.17 ± 0.32
29.1 109.400870 37.743174 1.7 ± 0.1, 1.7 ± 0.1, 1.7 ± 0.1 1.45 ± 0.07
29.2 109.392840 37.738612 1.62 ± 0.06
31.1 109.374720 37.756347 1.6 ± 0.1, 1.6 ± 0.1, 1.6 ± 0.1 1.55 ± 0.08
31.2 109.371000 37.750538 1.52 ± 0.06
31.3 109.381610 37.764973 1.57 ± 0.08
32.1 109.369500 37.757729 2.3 ± 0.1, 2.8 ± 0.1, 2.5 ± 0.1
32.2 109.380950 37.769382
32.3 109.366250 37.749210 2.40 ± 0.05
33.1 109.383770 37.758259 3.5 ± 0.3, 3.7 ± 0.2, 3.7 ± 0.1
33.2 109.386620 37.764144
33.3 109.370370 37.738712
34.1 109.391580 37.766308 2.6 ± 0.2, 2.7 ± 0.2, 2.6 ± 0.1
34.2 109.379110 37.751227 1.03 ± 0.05
34.3 109.373300 37.744211 1.11 ± 0.09
36.1 109.364330 37.771976 2.4 ± 0.2, 2.9 ± 0.2, 2.6 ± 0.1
36.2 109.358240 37.763325
36.3 109.353290 37.755808
37.1 109.397090 37.754736 3.8 ± 0.8, 3.3 ± 0.7, 3.3 ± 0.4
37.2 109.396720 37.754793
39.1 109.402270 37.731234 4.3 ± 0.3, 4.1 ± 0.3, 4.1 ± 0.3 1.82 ± 0.04
39.2 109.404950 37.732519 2.14 ± 0.19
39.3* 109.414740 37.743276
45.1 109.389820 37.739214 2.7 ± 0.1, 2.7 ± 0.1, 2.6 ± 0.1
45.2 109.383480 37.737879
45.3 109.404470 37.761960
49.1 109.402800 37.733260 >4.8, 4.1 ± 0.3, 3.8 ± 0.2 3.40 ± 0.08
49.2 109.393000 37.730812 3.54 ± 0.06
50.1 109.374440 37.743736 3.7 ± 0.4, 3.6 ± 0.3, 3.6 ± 0.2 3.19 ± 0.10
50.2 109.379580 37.750708
50.3* 109.392800 37.767181
52.1 109.368380 37.771761 3.0 ± 0.2, 3.3 ± 0.2, 3.3 ± 0.3
52.2 109.360230 37.760497
52.3 109.357040 37.752486
55.1 109.373760 37.755778 2.2 ± 0.1, 2.4 ± 0.1, 2.4 ± 0.1
55.2 109.370240 37.748743 2.17 ± 0.11
55.3 109.385020 37.768411
56.1 109.373150 37.744015 3.2 ± 0.2, 3.2 ± 0.2, 3.0 ± 0.1
56.2 109.378400 37.751095
56.3* 109.391820 37.766216
57.1 109.379030 37.744097 1.7 ± 0.1, 1.8 ± 0.2, 1.7 ± 0.1
57.2 109.379530 37.745110
58.1 109.379420 37.762383 4.2 ± 1.4, 4.2 ± 1.2, uncons. 3.03 ± 0.34
58.2 109.379260 37.762129
59.1 109.376840 37.743245 3.4 ± 0.8, 4.2 ± 0.5, 3.6 ± 0.5 3.11 ± 0.23
59.2 109.379960 37.748146
59.3* 109.400700 37.768628
62.1 109.372220 37.747464 2.7 ± 0.3, 2.9 ± 0.3, 2.7 ± 0.3 2.23 ± 0.08
62.2 109.375510 37.752276 2.23 ± 0.06
63.1 109.369420 37.756278 1.3 ± 0.1, 1.6 ± 0.1, 1.7 ± 0.1 2.20 ± 0.24
63.2 109.368360 37.753695 2.20 ± 0.18
64.1* 109.372250 37.765391
64.2* 109.371790 37.765066
65.1 109.383120 37.762595 5.4 ± 0.3, >4.6, >5.0
65.2 109.382250 37.760394
66.1 109.383310 37.765079 >6.5, 6.4 ± 0.8, 6.5 ± 0.4
66.2 109.380290 37.759228
67.1 109.367470 37.756509 3.0 ± 0.1, 4.2 ± 0.9, 4.5 ± 0.5
67.2 109.365120 37.749544
67.3* 109.382090 37.771629
68.1 109.392330 37.738083 5.51
68.2 109.382350 37.736508
68.3* 109.406780 37.763803
69.1 109.380400 37.749467 3.4 ± 0.5, 3.3 ± 0.4, 3.1 ± 0.4
69.2 109.375320 37.743383
69.3* 109.396440 37.768591
70.1 109.392210 37.760496 3.7 ± 0.4, 3.1 ± 0.2, 3.9 ± 0.3 2.72 ± 0.06
70.2 109.389380 37.757279 3.11 ± 0.07
70.3* 109.375110 37.735945 2.14 ± 0.09
71.1 109.382700 37.744711 3.0 ± 0.1, 2.6 ± 0.1, 2.6 ± 0.1 2.91 ± 0.10
71.2 109.380650 37.741346 1.82 ± 0.04
71.3 109.402550 37.763610 2.65 ± 0.16
71.4 109.387210 37.741295
72.1 109.380120 37.765496 >4.1, >4.0, 3.9 ± 0.4 3.32 ± 0.14
72.2 109.374810 37.762346 3.32 ± 0.22
73.1* 109.375970 37.748883
73.2* 109.375500 37.748483
73.3* 109.391470 37.767033
74.1* 109.370890 37.751182 1.52 ± 0.06
74.2* 109.383420 37.769708
74.3* 109.371310 37.751974 1.60 ± 0.15
75.1 109.382000 37.738429 3.6 ± 0.4, 4.7 ± 0.4, 4.3 ± 0.5
75.2 109.388640 37.739263
75.3* 109.40496 37.764678
76.1 109.411230 37.731990 4.5 ± 0.4, 5.4 ± 0.3,3.7 ± 0.4
76.2 109.412840 37.733789
76.3 109.413660 37.734646
77.1* 109.377000 37.736456
77.2* 109.386260 37.751928
77.3* 109.399110 37.764959
78.1* 109.371840 37.742478
78.2* 109.379010 37.752778
79.1 109.393150 37.762795 3.7 ± 0.3, 3.4 ± 0.2,3.7 ± 0.3
79.2 109.387350 37.755963
79.3 109.375740 37.735628
80.1 109.390940 37.733628 3.7 ± 0.3, 3.3 ± 0.1, 3.8 ± 0.2 2.37 ± 0.15
80.2 109.400250 37.738496 2.50 ± 0.11
80.3 109.410080 37.753576 2.40 ± 0.14
81.1* 109.408320 37.728127
81.2* 109.409010 37.728544
81.3* 109.410160 37.729344
82.1* 109.383660 37.766146 2.65 ± 0.48
82.2* 109.379500 37.756303 2.72 ± 0.21

Notes. Images with Uncertainties quoted for redshifts predicted by our model, zmodel, correspond to the 1σ confidence level. They are given for the non-cored, the cored, and the NFW model. uncons means unconstrained, i.e. when the output PDF is flat. In the last column, we show the estimate of the photometric redshift, when possible, together with the 1σ error bars.

(*)

are the ones we propose as candidates and that are not used as constraints in the mass model.

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