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Fig. 1

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From left to right: observations, best fit model, and residuals, for the SPHERE and ALMA observations (top and bottom, respectively). The scaling is linear and the same for all horizontal panels. For the ALMA observations, the beam is shown in the leftmost panel, and the contours on the right panel are at [–1,1,2] σ (σ = 0.3 mJy beam−1).

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