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Table 3.
MACS 0416 results: non cored model.
| Non cored model | Δ RA | Δ Dec | e | θ | σ | rcore |
|---|---|---|---|---|---|---|
| (″) | (″) | (km s−1) | (kpc) | |||
| Clump 1 | −1.1 ± 0.3 | −0.1 ± 0.2 | 0.7 ( * ) | 135.4 ± 0.6 | 522 ± 4 | 10 ( * ) |
| Clump 2 | 21.6 ± 0.2 | −37.4 ± 0.4 | 0.7 ( * ) | 129.6 ± 0.8 | 651 ± 5 | 10 ( * ) |
| Clump 3 | −32.1 ± 0.1 | 12.9 ± 0.1 | 0.27 ± 0.08 | 126.5 ± 9.0 | 357 ± 8 | 10 ( * ) |
Notes. Same as Table 2 for the non cored model of MACS 0416, with an rms equal to 1.88″. For an L* galaxy, we have σ = 240 ± 5 km s−1 and rs = 108 kpc (stuck to the upper bound of the allowed prior).
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