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Table 2
Median values and confidence levels of the cluster total mass distribution parameters from the MCMC analysis of the strong lensing model.
| Median | 68% CL | 95% CL | 99.7% CL | |
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| Halo around BCG-North (relative position = (0″,0″)) | ||||
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| x1 (″) | − 2.4 |
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| y1 (″) | 1.8 |
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| ε 1 | 0.85 |
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| θ1 (deg) | 143.9 |
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| rcore,1 (″) | 6.3 |
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| σv1 (km s-1) | 707 |
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Halo around BCG-South (relative position =  ) |
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| x2 (″) | 19.6 |
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| y2 (″) | − 36.4 |
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| ε 2 | 0.77 |
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| θ2 (deg) | 125.6 |
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| rcore,2 (″) | 12.5 |
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| σv2 (km s-1) | 1102 |
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| Third spherical halo | ||||
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| x3 (″) | − 34.4 |
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| y3 (″) | 7.9 |
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| rcore,3 (″) | 6.4 |
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| σv3 (km s-1) | 434 |
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| Galaxy scale system 14 | ||||
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| εG1 | 0.3 |
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| θG1 (deg) | 115 |
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143 |
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8.1 |
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48 |
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5.2 |
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| Sub-halo population | ||||
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10.5 |
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251 |
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Notes. Coordinates are relative to the position of the BCG, N (RA = 04:16:09.15 and Dec = −24:04:03.0).
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