Table 6.
Relaxing the B19 priors.
| Model | rs | σ | rms | Δ(rms) |
|---|---|---|---|---|
| (kpc) | (km s−1) | (″) | (″) | |
| AS 1063, cored | 150 (43) | 230 (302) | 0.64 (0.67) | 3.07 (3.16) |
| AS 1063, non cored | 5 (5) | 100 (303) | 3.71 (3.83) | – |
| MACS 0416, cored | 42 (10) | 264 (237) | 0.62 (0.63) | 1.18 (1.44) |
| MACS 0416, non cored | 42 (10) | 201 (237) | 1.80 (2.07) | – |
| MACS J1206, cored | 29 (41) | 295 (266) | 0.52 (0.53) | 1.81 (6.83) |
| MACS J1206, non cored | 150 ( * ) (92) | 297 (253) | 2.33 (7.49) | – |
Notes. Results obtained on the galaxy scale perturbers when relaxing the B19 priors, for the different models explored. We also report the rms obtained and the difference of rms between the non cored and the cored mass model. Values into brackets correponds to the results obtained when considering the B19 priors. Parameters with ( * ) are stuck to a bound of the allowed prior.
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