Fig. C.1.
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Highest-likelihood EPL lens models for alternative datasets. Each row illustrates a different assumption for the noise added to empty regions. From left to right: Model image, normalized residuals, and reconstructed source. Top row: Dataset where the modified image uses a σ10 dispersion. Bottom row: σ20 dispersion. Fluxes are in units of 10−18 erg s−1 cm−2.
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