Fig. E.2

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Resulting radiative transfer images from our 3D (upper panels) and 2D (lower panels) hydrodynamical simulations for the planets described in Fig. E.1. The mass and separation increase from left to right. The images have been processed with the same techniques as the ones in Fig. 8 for a better comparison to the observations. For the lower panels, we show the images that fit the inner spirals.
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