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Table A.1.

Lens model parameters used to create the baseline datasets.

Lens system REin gx gy ϵ θϵ γ γext θext R1 x1 y1 z1 R2 x2 y2 z2
RXJ1131−1231 1.58 −0.01 −0.03 0.14 34 1.98 0.12 −82 0.28 −0.1 0.61 zd
PG1115−080 1.05 0.0 0.0 0.01 −71 2.20 0.03 −56 2.0 −9.21 −3.91 zd
HE0435−1223 1.17 −0.02 0.02 0.07 −81 1.98 0.05 10 0.35 −2.27* 1.98* zd + 0.33
B1608+656 0.90 0.01 0.06 0.51 −4 2.08 0.10 26 0.26 −0.71 0.13 zd
WFI2033−4723 1.0 −0.02 0.02 0.22 57 1.95 0.17 −8 0.03 0.24 2.04 zd 0.93 −3.63* −0.68* zd + 0.09
DESJ0408−5354 1.72 0.14 0.00 0.39 23 1.92 0.11 5 0.22 −1.58 −0.95 zd 0.77 1.13* −7.45* zd + 0.17

Notes. The main deflector is modeled as an elliptical power law plus external shear, and other satellites or field galaxies are modeled with spherical power law profiles. Parameters from left to right: Einstein radius of the main deflector, x and y mass centroid of main deflector, main deflector ellipticity and position angle, logarithmic slope of the main mass profile, external shear magnitude and position angle. The columns labeled Ri, xi, yi, zi contain the Einstein radii, coordinates, and redshifts of satellite galaxies, or galaxies along the line of sight, that are included in the mock lens models. Angular positions marked with an asterisk indicate that this coordinate is corrected for foreground lensing effects by the main deflector.

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