Table B.1.
Input parameters and results of the GravLens model fitting of the lens.
Input parameters | ||||
---|---|---|---|---|
Cosmology | Ωm, ΩΛ | 0.3, 0.7 | ||
H0 (km s−1 Mpc−1) | 67.4 ± 0.5; ![]() |
(1) | ||
Source | Redshift zS | 2.507 | (2) | |
Intensity profile | Point-like | |||
Lens | Redshift zL | 0.88582 | (3) | |
Initial guess position | −500.1, −459.6 | (4) | ||
Mass distribution | Softened isothermal ellipsoidal | |||
Lensed images | Position of image A | (ΔRA, ΔDec) ≡ (0, 0) | (5) | |
Position of image B (mas) | −641.946 ± 0.042, −728.082 ± 0.033 | (6) | ||
Position of image C (mas) | −500.1 ± 2.1, −459.6 ± 1.6 | (6) | ||
Flux ratios (A:B:C) | 1 : 0.93 ± 0.09 : 0.0071 ± 0.0009 | (7) | ||
Output parameters | ||||
Best fit | Guess range | |||
Source | Position xs, ys (mas) | −386 ± 3, −325 ± 2 | (8) | |
Flux fs |
![]() |
(9) | ||
Lens | Position xl, yl (mas) | −489 ± 2, −444 ± 2 | (8) | |
Mass scale (mas) | 505 ± 6 | [100; 1500] | (10) | |
Softening length s (mas) | 26 ± 2 | [10; 200] | (10) | |
Ellipticity e | 0.19 ± 0.02 | [0.0; 0.3] | ||
Position angle θ (°) |
![]() |
[−90;+90] | ||
Derived quantities | ||||
Time delay | tAB (d) | 28.6; 26.3 | (11) | |
tAC (d) | 33.7; 31.0 | (11) | ||
Magnification | μA | 3.1 | ||
μB | −2.9 | |||
μC | 0.022 |
Notes. (1) H0 measurements from Planck Collaboration VI (2020) and Wong et al. (2020), respectively. (2) Lidman et al. (1999). (3) Wiklind & Combes (1996). (4) Set as image C (Table 1), as both are expected to be very close in the plane of the sky. (5) Taken as position reference. (6) Positions from this work (Table 1) given with respect to image A. (7) Flux ratios from this work (Table 1). (8) Positions relative to image A. (9) Flux of the source normalized to that of image A (i.e., inverse of the magnification, fs = 1/μA). (10) As defined in Eq. (B.5). (11) Time delays corresponding to H0 values of 67.4 km s−1 Mpc−1 and 73.3 km s−1 Mpc−1, respectively.
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