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Table 2.

Input and optimized output parameter values of the reference model.

Input parameter values and intervals of reference lens model
x [arcsec] y [arcsec] e θ [°] σLT [km s−1] rcore [arcsec] rcut [arcsec]
Main DM Halo −3.0 ÷ 3.0 −3.0 ÷ 3.0 0.0 ÷ 0.3 −40.0 ÷ 40.0 800.0 ÷ 1100.0 2.0 ÷ 15.0 2000.0
Nord DM Halo −16.0 ÷ 0.0 10.0 ÷ 34.0 0.0 ÷ 0.9 −90.0 ÷ 90.0 300.0 ÷ 800.0 0.01 ÷ 15 2000.0

1678 0.72 34.72 0.0 0.0 30.0 ÷ 120.0 0.01 0.1 ÷ 15.0
1677 5.04 33.0 0.0 0.0 50.0 ÷ 150 0.01 0.1 ÷ 20.0
N-ARC R 8.07 29.91 0.0 ÷ 0.9 0.0 ÷ 140.0 10.0 ÷ 150.0 0.01 0.0 ÷ 20.0
BK N-NW 12.31 25.96 0.0 0.0 30.0 ÷ 150.0 0.01 0.1 ÷ 15.0
BK NW L 12.0 ÷ 16.0 22.0 ÷ 26.0 0.0 ÷ 0.9 −90.0 ÷ 90.0 10.0 ÷ 200.0 0.01 0.1 ÷ 15.0
1298 19.0 14.71 0.6 ÷ 0.9 0.0 ÷ 180.0 10.0 ÷ 200.0 0.01 0.0 ÷ 15.0

Scaling relations Ngal = 194 = 17.71 α = 0.31 180.0 ÷ 280.0 βcut = 0.57 0.1 ÷ 25.0 γ = 0.2

Optimized output parameters of reference lens model
x [arcsec] y [arcsec] e θ [°] σLT [km s−1] rcore [arcsec] rcut [arcsec]

Main DM Halo 2000.0
Nord DM Halo 2000.0

1678 0.72 34.72 0.0 0.0 0.01
1677 5.04 33.0 0.0 0.0 0.01
N-ARC R 8.07 29.91 0.01
BK N-NW 12.31 25.96 0.0 0.0 0.01
BK NW L 0.01
1298 19.0 14.71 0.01

Scaling relations Ngal = 194 = 17.71 α = 0.31 βcut = 0.57 γ = 0.2

Notes. Top: input parameter values of the reference model. The single numbers are fixed parameters, while for the free parameters we report the lower and upper limits of the input flat priors. In the last row, we report the input parameters for the scaling relations used to parametrize the subhalo component. Bottom: output parameter values from the optimization of the reference model. We report the median value of the parameter with errors corresponding to the [16th, 84th] percentiles of the marginalized posterior distribution.

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