Table 2.
Recovered properties of potential perturbations, from the MAP ψpix models shown on Fig. 5.
| Lens | Parameters | Input values | Model | Measured values |
|---|---|---|---|---|
| LS | (θx, sub, θy, sub) | (1.90, −0.40) | Pixelated | (1.94 ± 0.12, −0.49 ± 0.12) |
| Refined | (1.899 ± 0.008, −0.408 ± 0.005) | |||
| log10Msub | 8.91 | Pixelated | 8.71 ± 0.05 | |
| Refined | 8.90 ± 0.01 | |||
| Pixelated, ideal | ( − 3.35 ± 0.20, 3.40 ± 0.15) | |||
| PS |  |
( − 3.11 ± 0.15, 3.23 ± 0.05) | Pixelated, fiducial | ( − 3.89 ± 0.25, 4.15 ± 0.19) |
| Pixelated, high-res | ( − 3.49 ± 0.15, 3.26 ± 0.09) | |||
| HM | (am, ϕm) | (0.06, 82.50) | Pixelated | (0.024 ± 0.002, 83.78 ± 0.88) |
| Refined | (0.061 ± 0.002, 83.15 ± 0.39) | |||
| m | 4 | Refined | 4.01 ± 0.02 | |
Notes. The quoted values for the subhalo mass is given in solar units and computed within the region with S/N(ψpix) > 3 (see Fig. 8 and text for more details). The input GRF parameters are given with uncertainties as they were fitted on the power-spectrum of the input perturbing field.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.