Fig. A.1
Qφ (left) and Uφ (middle) images of model #1 at H-band. The right panel considers the same model, but the star is slightly offset from its original central position along the semi-major axis. The images are convolved with a Gaussian PSF with FWHM of 0.̋04 (at 107 pc distance). The color scale considers the same dynamical range as for the previous synthetic images.
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