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Fig. 4

Fig. 4 Refer to the following caption and surrounding text.

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Left: Qϕ image of WRAY 15-1880 obtained from the SPHERE polarimetric data. The red dot at the center of the image marks the position of the star; the position of the candidate planet at the epoch of the SPHERE polarimetric observation is marked with a small magenta circle. Middle: scattering model considered for the disk (see text). Right: residuals

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