Notes. In addition to enlisting the system names in DESI’s decimal convention, we also provide their alternative sexagesimal version (in parentheses). The description of each model setting is described in Section 3. The contributing modelers for each system are also tabulated. For some systems, we have imposed a prior condition on the satellite galaxy’s Einstein radius for it to scale with the mass, assuming the mass-to-light ratio is the same for both the central deflector and the satellite. This condition is denoted with ${\theta }_{\mathrm{E},\mathrm{Cen}}/{\theta }_{\mathrm{E},\mathrm{Sat}}=\sqrt{{\mathrm{flux}}_{\mathrm{Cen}}/{\mathrm{flux}}_{\mathrm{Sat}}}$ for the cases it was used.