Fig. 2

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Left: close up of the final Qϕ SPHERE/IRDIS-DPI image after removing low frequency structures (see text for details) and applying a Gaussian kernel of size 0.1 × FWHM to smooth the images and enhance the spiral features. Right: close up of the final Uϕ image showing the positive and negative signal. The 93 mas coronagraph is indicated by the gray circle, and the cross indicates the position of the star. The flux is normalized to the maximum value in the Qϕ image.
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