Table A.2.
dPIE parameters inferred for our best model of MACS 0416.
| ΔRA | ΔDEC | e | θ | σ (km s−1) | rcore (kpc) | |
|---|---|---|---|---|---|---|
| Main Clump | -2.6±0.7 (-1.8) | 1.7±0.5 (1.2) | 0.78±0.02 (0.76) | 144±1 (143) | 600±19 (612) | 42.2±3.2 (42.7) |
| South Clump | 22.0±0.4 (22.3) | -39.1±0.6 (-39.4) | 0.72±0.02 (0.70) | 126±1 (126) | 806±16 (795) | 59.8±3.2 (57.9) |
| NE Clump | -32.6±1.4 (-31.7) | 9.0±1.4 (9.0) | 0.25±0.1 (0.24) | 104±21 (99) | 338±40 (358) | 42.2±13.3 (45.8) |
Notes. The RMS for our best fit model equals to 0.57″, obtained with (RATE, Nb) = (0.005, 5000). Coordinates are given in arcseconds relative to α = 64.0382167, δ = -24.0675012; e and θ are the ellipticity and position angle of the mass distribution. Each parameter is given as the median (± 1σ confidence level) with the best fit value in parentheses. For an L* galaxy, we have σ = 208±8 km s−1 and rs = 15.0±2.3" kpc.
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