Fig. B.1
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Real (top panel) and imaginary (bottom panel) parts of the re-centred and de-projected visibilities azimuthally averaged in bins with width of 20 kλ as a function of the de-projected baseline length for HD 34700A (left), IRS 48 (middle) and HD 142527 (right). The black points represent the visibility data points, while the red solid line corresponds to the galario best fit model.
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