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Table 4

Multiply-imaged systems used to constrain the model, with their ID, centroid position, brightness, colors, linear magnification and predicted or spectroscopically measured redshifts.

System RA Dec F606W F606WF775W F775WF850LP F850LPF110W F110WF160W μ zphot zspec
(deg) (deg)

Main Clump

A.1 104.63293 –55.941725 25.59 ± 0.07 0.64 ± 0.09 0.02 ± 0.09 0.13 ± 0.08 0.41 ± 0.05 29.56 ± 8.97 3.24
A.2 104.63158 –55.942454 25.65 ± 0.05 0.51 ± 0.09 0.09 ± 0.09 0.21 ± 0.07 0.42 ± 0.04 26.22 ± 6.68
A.3 104.63055 –55.943405 25.67 ± 0.06 0.66 ± 0.11 0.02 ± 0.09 0.02 ± 0.08 0.37 ± 0.06 12.48 ± 0.90
Fa.1b 104.65210 –55.956245 24.63 ± 0.06 0.30 ± 0.08 −0.07 ± 0.09 0.15 ± 0.08 0.42 ± 0.05 9.77 ± 0.44 2.14 ± 0.19
Fa.2 104.64704 –55.958497 24.12 ± 0.05 0.22 ± 0.03 −0.08 ± 0.03 0.18 ± 0.03 0.41 ± 0.05 11.11 ± 0.72
Fa.3 104.66515 –55.951289 25.33 ± 0.11 0.37 ± 0.15 −0.01 ± 0.15 0.08 ± 0.14 0.52 ± 0.09 4.89 ± 0.22
Fb.1b 104.65165 –55.956641 25.31 ± 0.09 0.30 ± 0.08 −0.07 ± 0.09 0.14 ± 0.08 0.39 ± 0.08 14.91 ± 1.11
Fb.2 104.64786 –55.958292 25.09 ± 0.12 0.24 ± 0.04 −0.03 ± 0.04 0.06 ± 0.04 0.13 ± 0.10 15.02 ± 0.96
Fb.3 104.66544 –55.951301 26.61 ± 0.36 0.45 ± 0.11 −0.08 ± 0.11 0.04 ± 0.10 0.27 ± 0.09 4.77 ± 0.21
E.1 104.64242 –55.948720 25.52 ± 0.05 0.49 ± 0.08 0.11 ± 0.07 0.15 ± 0.06 0.43 ± 0.08 15.96 ± 1.36 3.17 ± 0.27
E.2 104.63954 –55.951165 25.51 ± 0.04 0.55 ± 0.08 0.22 ± 0.06 0.11 ± 0.05 0.37 ± 0.05 16.72 ± 1.30
E.3 104.65434 –55.944392 25.77 ± 0.04 0.45 ± 0.07 0.33 ± 0.06 0.20 ± 0.05 0.42 ± 0.06 7.13 ± 0.40
K.1 104.65864 –55.950557 2.79
K.2 104.65459 –55.951876
K.3 104.63929 –55.958032
1.1 104.65049 –55.953339 27.20 ± 0.13 0.25 ± 0.17 0.19 ± 0.25 0.89 ± 0.18 0.17 ± 0.04 15.65 ± 1.20 1.21 ± 0.23
1.2 104.64572 –55.955109 26.83 ± 0.11 0.29 ± 0.09 0.30 ± 0.07 0.50 ± 0.05 0.24 ± 0.05 11.20 ± 0.57
1.3* 104.65706 –55.950866
2.1 104.65560 –55.948760 25.62 ± 0.06 0.32 ± 0.21 0.27 ± 0.26 0.21 ± 0.21 0.51 ± 0.11 10.61 ± 0.40 2.91 ± 0.25
2.2 104.65203 –55.950014 24.59 ± 0.06 0.56 ± 0.12 0.24 ± 0.09 0.21 ± 0.08 0.49 ± 0.05 14.18 ± 0.94
2.3 104.63801 –55.956311 26.35 ± 0.07 0.45 ± 0.16 0.44 ± 0.13 0.25 ± 0.10 0.57 ± 0.08 4.79 ± 0.21
3.1 104.65770 –55.948271 24.74 ± 0.05 0.61 ± 0.18 −0.01 ± 0.07 −0.09 ± 0.05 0.23 ± 0.02 9.37 ± 0.54 4.06 ± 1.23
3.2 104.65118 –55.950472 26.74 ± 0.08 0.95 ± 0.32 −0.22 ± 0.17 −0.26 ± 0.15 0.38 ± 0.12 4.73 ± 0.14
3.3 104.63565 –55.957061 >28.50 >1.51 −0.34 ± 0.07 −0.05 ± 0.27 0.53 ± 0.24 4.94 ± 0.22
4.1 104.64423 –55.949050 27.58 ± 0.38 0.21 ± 0.12 0.57 ± 0.04 −0.29 ± 0.04 −0.08 ± 0.05 22.96 ± 2.11 2.00 ± 0.12
4.2 104.64251 –55.950576 26.97 ± 0.28 0.28 ± 0.14 0.36 ± 0.07 −0.33 ± 0.05 −0.20 ± 0.04 20.04 ± 1.71
4.3* 104.65166 –55.944823
5.1 104.64961 –55.947382 27.44 ± 0.23 1.14 ± 0.21 −0.72 ± 0.19 −0.06 ± 0.17 0.26 ± 0.35 4.70 ± 0.20 2.54 ± 0.34
5.2 104.64928 –55.947412 27.56 ± 0.45 0.90 ± 0.18 −0.31 ± 0.12 −0.40 ± 0.10 0.21 ± 0.26 4.75 ± 0.20
5.3* 104.63731 –55.953223
D.2 c 104.63981 –55.947308 26.56 ± 0.20 −0.19 ± 0.08 0.02 ± 0.06 0.41 ± 0.04 0.27 ± 0.01 49.83 ± 10.34
D.1 104.63943 –55.947552 26.79 ± 0.24 −0.31 ± 0.14 −0.13 ± 0.16 0.80 ± 0.10 0.36 ± 0.02 50.19 ± 5.42 3.23 ± 0.42
D.3 104.64623 –55.944115 25.52 ± 0.22 −0.03 ± 0.07 0.17 ± 0.06 0.57 ± 0.03 0.32 ± 0.01 49.96 ± 3.23

Notes. The systems and their properties, along with references to the papers reporting their redshifts, are given in Sect. 3. Images marked * are not detected, thus their positions are just predictions from lens model. We do not report photometry on system K since it is smm galaxy, invisible in ACS/HST. Numbers (.1, .2 , etc.) denote the different images of each set of multiple images. Each multiple image is presented in Fig. 5, except system K that is invisible in optical and system D that has not been included in the model optimization is presented in Fig. 7.

(a)

Redshift estimation inferred from the mass model when all spectroscopically confirmed multiply-imaged systems have been included in the optimization.

(b)

System Fa and Fb are most probably gravitationally bounded.

(c)

System D is not included in the model optimization, it is a multiply-imaged candidate.

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