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Table 5

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

System RA Dec F606W F435WF606W F606WF814W F435WF814W μ zphot zspec
(deg) (deg)

Sub clump

H.1 104.56305 –55.939755 26.59 ± 0.08 0.65 ± 0.11 −0.21 ± 0.07 0.43 ± 0.12 6.48 ± 0.67 2.99
H.2 104.56145 –55.942423 26.78 ± 0.08 0.78 ± 0.14 −0.40 ± 0.09 0.36 ± 0.16 9.62 ± 0.87
H.3 104.56202 –55.947717 26.57 ± 0.12 1.00 ± 0.15 −0.29 ± 0.06 0.29 ± 0.14 11.74 ± 1.53
I.1n 104.56478 –55.938146 26.36 ± 0.14 0.47 ± 0.11 0.17 ± 0.07 0.64 ± 0.11 5.31 ± 0.50
I.2 104.56155 –55.944252 25.55 ± 0.07 0.50 ± 0.07 0.08 ± 0.04 0.59 ± 0.07 20.25 ± 3.38 3.24 ± 0.13
I.3 104.56192 –55.946101 25.60 ± 0.05 0.49 ± 0.06 0.03 ± 0.04 0.52 ± 0.06 15.91 ± 1.53
J.1 104.57038 –55.944036 26.81 ± 0.13 −0.11 ± 0.08 −0.47 ± 0.09 −0.58 ± 0.10 24.49 ± 4.01 2.02 ± 0.25
J.2 104.56917 –55.946003 27.03 ± 0.12 −0.32 ± 0.10 −0.19 ± 0.10 −0.50 ± 0.11 19.33 ± 1.99
J.3 104.56993 –55.938772 27.99 ± 0.55 −0.17 ± 0.21 −0.37 ± 0.16 −0.20 ± 0.18 5.39 ± 0.48
G.1 104.56580 –55.939857 25.31 ± 0.05 > 1.85 0.40 ± 0.05 > 2.25 11.60 ± 1.56 0.73 ± 0.09
G.2 104.56424 –55.941963 25.27 ± 0.06 >1.73 0.57 ± 0.06 >2.16 13.46 ± 1.04
G.3n* 104.56471 –55.947724
6.1 104.56406 –55.945386 26.05 ± 0.08 −0.14 ± 0.09 0.25 ± 0.07 0.11 ± 0.08 40.90 ± 4.88 2.51 ± 0.12
6.2 104.56384 –55.944904 26.17 ± 0.11 −0.08 ± 0.09 0.15 ± 0.08 0.07 ± 0.09 31.30 ± 5.68
6.3* 104.56627 –55.938208 >28.45 4.86 ± 0.43
7.1b 104.56084 –55.946952 26.89 ± 0.15 0.07 ± 0.35 −0.36 ± 0.45 −0.29 ± 0.23 22.71 ± 3.39 3.00 ± 0.19
7.2 104.56054 –55.942898 26.54 ± 0.12 0.15 ± 0.22 0.03 ± 0.32 0.18 ± 0.13 16.79 ± 1.90
7.3 104.56230 –55.939588 26.89 ± 0.13 0.03 ± 0.34 0.25 ± 0.29 0.28 ± 0.38 10.94 ± 0.78

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. Numbers (.1, .2 , etc.) denote the different images of each set of multiple images, each presented in Fig. 6, except system 7 that has not been included in the model optimization.

(a)

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

(b)

System 7 is not included in the model optimization, it is multiply-imaged candidate.

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