Fig. B.1.

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Joint posterior PDFs for the model Esr2-3MP based on two extended sources and image positions. We show the parameters representing the lens masses at three multiple planes. The θE, GH and θE, BGG are the Einstein radius of the group halo and the BGG at the main lens plane at z = 0.683. The xz = 1.36 and yz = 1.36 are the centroid of the perturber, and the θE, z = 1.36 is its Einstein radius. The θE, S0 is the Einstein radius of S0 at z = 1.49. The three shaded areas on the joint PDFs show the 68.3%, 95.4%, and 99.7% credible regions. The 1D histograms show the marginalized PDFs for the selected mass parameters, and the vertical lines mark the 1σ confidence intervals. The θE, S0 shows strong degeneracies with θE, BGG, θE, GH, and θE, z = 1.36.
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