Fig. 9.
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Reconstructed image of HE 1104−1805 using the best power-law and composite models. From left to right: The imaging data, reconstructed image, and normalised residuals are displayed for the power law model (PEMD + Shear + perturbers 2, 5, 6, 9 + groups 1, 2, 3, and 4) and composite models (NFW + Double chameleon + Shear + perturbers 2, 5, 6, 9 + groups 1, 2, 3, and 4).
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