Fig. A.2.

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Removal of scattered light contamination produced by bright stars near AGC 114905. The panels illustrate the procedure followed in the g-band data. The left and middle panels show the original stacked image and the model of the scattered light, respectively. Our final science images are the result of subtracting the model from the original image, as displayed in the right panel. The field of view of the region is 5 arcmin × 5 arcmin.
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