Fig. 4
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One panel for the response method expanded over the full shear range of the fit methods from −0.1 to 0.1. The legend above indicates the applied shear g1 for each stamp. The shear difference Δg is 0.02 from stamp to stamp. One can observe the virtually identical noise pattern in each stamp, which only differs due to the Poisson noise of the galaxy itself as described in Sect. 3.2.
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