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Fig. B.1.


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True versus predicted Kron magnitudes mF160W plots (upper panel) and residuals (lower panel) for 222 spectroscopic cluster members. The predicted values were obtained using two linear regressors trained using Kron magnitudes, mF110W and mF814W, (red and blue points, respectively). The brown dash-dotted line indicates the magnitude threshold used to select the cluster members sample used for the strong-lensing model. The table shows various statistical indicators for the best and worst regressor, considering all the values (first and third column) or only the objects for which mF160W ≤ 21 (second and last column).

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