Table B.1.
Overview of the lens mass models from the seven independent modeling approaches using the gold image positions as constraints.
| Description | GLAFIC | GLEE | GLEE -baseline | Lenstool I | Lenstool II | ZITRIN-ANALYTIC | MrMARTIAN | WSLAP+ |
|---|---|---|---|---|---|---|---|---|
| BCG profile | Hernquist | dPIE | dPIE | dPIE | dPIE | dPIE | — (hybrid) | — (free-form) |
| Number of DM halos | 1 | 2 | 2 | 1 | 1 | 2 | 1 + grid | — (free-form) |
| DM halo profile | NFW | variousa | isothermal | dPIE | dPIE | isothermal | NFW + grid | — (free-form) |
| External shear | Yes | No | No | Yes | Yes | No | — | — |
| Galaxy scaling relation | ||||||||
| α | 0.25 | 0.25b | 0.25b | 0.25 | 0.21b | 0.25 | — | — |
| β | 0.5 | 0.7 | 0.7 | 0.5 | 0.71 | 0.5 | — | — |
| Galaxies not in scaling relation | fg, JF-1 | multiplec | multiplec | multipled | multiplee | multiplef | — | — |
| positional error boost factor | 1 | 1 | 1 | 2.2 | 1.5 | 3 | 1 | 1 |
Notes.
Various halo profiles were explored, including isothermal, power-law and NFW; one model also included a mass sheet.
The parameter α of the scaling relation (Eq. 1) was optimized using cluster member galaxies with velocity dispersion measurements in the GLEE (Granata et al. 2025; Ertl et al. 2025) and LENSTOOL II (Acebron et al. 2025) models, whereas α was fixed to the tabulated values in the other models.
The multiple objects excluded from the galaxy scaling relation of the GLEE model are: BCG, object ID = 116, JF-1, JF-2, JF-3, fg, and bg (see Ertl et al. 2025).
The multiple objects excluded from the galaxy scaling relation of the LENSTOOL I model are: object at (RA, Dec) =
, JF-1, JF-2, JF-3, and fg.
The multiple objects excluded from the galaxy scaling relation of the LENSTOOL II model are: JF-1, JF-2, JF-3, fg, and bg.
Four objects excluded from the galaxy scaling relation of the ZITRIN-ANALYTIC model are located at (RA, Dec) =
,
,
, and
.
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