Table 5.
DV+NFW+ES lens models.
| f* | κ |
κ*/κ |
γ |
μ |
ΔtAB (d) | ||||
|---|---|---|---|---|---|---|---|---|---|
| A | B | A | B | A | B | A | B | ||
| 0.1 | 0.67 | 0.90 | 0.02 | 0.05 | 0.30 | 0.35 | 52.1 | 9.1 | 22.7 |
| 0.2 | 0.62 | 0.86 | 0.05 | 0.11 | 0.34 | 0.45 | 31.7 | 5.5 | 27.7 |
| 0.3 | 0.73 | 0.84 | 0.07 | 0.17 | 0.23 | 0.40 | 42.7 | 7.5 | 21.5 |
| 0.4 | 0.65 | 0.79 | 0.10 | 0.24 | 0.29 | 0.52 | 25.1 | 4.4 | 28.1 |
| 0.5 | 0.57 | 0.73 | 0.14 | 0.32 | 0.36 | 0.65 | 16.3 | 2.9 | 34.6 |
| 0.6 | 0.48 | 0.68 | 0.20 | 0.42 | 0.42 | 0.77 | 11.5 | 2.0 | 41.1 |
| 0.7 | 0.40 | 0.63 | 0.28 | 0.52 | 0.49 | 0.90 | 8.5 | 1.5 | 47.6 |
| 0.8 | 0.32 | 0.58 | 0.40 | 0.65 | 0.56 | 1.02 | 6.6 | 1.2 | 54.2 |
| 0.9 | 0.24 | 0.52 | 0.60 | 0.81 | 0.62 | 1.15 | 5.2 | 0.9 | 60.7 |
| 1.0 | 0.16 | 0.47 | 1.00 | 1.00 | 0.69 | 1.27 | 4.3 | 0.7 | 67.2 |
Notes. The ten lens models fit the observational constraints with χ2 ∼ 0 (d.o.f. = 0; see main text). The parameter f* represents the luminous mass of G relative to that for the model without dark matter halo (f* = 1). We list the convergence (κ), stellar to total convergence ratio (κ*/κ), shear (γ), and macrolens magnification (μ) for each model and image position. The last column shows the predicted time delay between images for each model.
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