Fig. A.2.
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Spaxels cleaned for wiggles (within the regions enclosed with white borders). Only the spaxels within a circle of
radius from the lens galaxy center were considered to be cleaned. Then, we only cleaned the spaxels for which the wiggle was detected at a confidence level of more than 3σ and the best-fit wiggle model explains more than half of the variance or scatter observed in the wiggle signal. The wiggles are more prominent in spaxels with more flux. As a result, the white contours above primarily encompass the central region of the lens galaxy and the satellite galaxy.
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