Fig. A.2

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Flux calibrated stacked total intensity image. We note that in this image the stellar light was not removed. The bright ring visible on the outer edge of the image shows the adaptive optics correction radius which shows bright stellar speckle signal (smoothed out by the field rotation during observations). The signal of the disk is faintly visible close to the coronagraph. The image is shown on a (logarithmic) scale, symmetric around 0. The grey, hashed circle in the center marks the area that was covered by a coronagraphie mask.
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