Table 4
Illustration of the implication of the systematic uncertainty on magnification estimates.
| ID | Ampli (cored) | Ampli (non-cored) | Δ [cored – noncored] | Δ [pre-HFF] |
|
|
||||
| 19.3 | 3.2 ± 0.15 [21] | 2.8 ± 0.07 [40] | 0.4 | 1.7 |
| 68.2 | 24 ± 2.0 [12] | 8.7 ± 0.6 [14.5] | 15.3 | 4.0 |
| 71.2 | 12.0 ± 1.4 [8.5] | 10.0 ± 0.7 [14] | 2.0 | 63.5 |
| 61.2 | 2.3 ± 0.2 [11.5] | 1.6 ± 0.1 [16] | 0.7 | 1.62 |
| 57.1 | 12.3 ± 6.0 [2] | 32.4 ± 846 [<1] | > 100 | 205 |
| 23.2 | 1083 ± 9167 [<1] | 21.8 ± 2.5 [<1] | > 1000 | 69 |
Notes. For different multiple images, the value of the amplification with associated errors and signal-to-noise ratio (in brackets), for the cored and the non-cored model; the difference in amplification between the cored and the non-cored mass model; the difference in amplification considering pre-HFF data and the different modelling/group software. Magnifications computed for z = 3.0.
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