Dust density distribution at different times of evolution (upper row) and the corresponding real part of the visibilities at λ = [0.87,1.0,3.0,7.0] mm (lower row) at different times of dust evolution, when a 20 M_Jup planet (left column) and 30 M_Jup planet (right column) is embedded in the inner disk. Data from ALMA Cycle 0 from Walsh et al. (2014) and ATCA from Wright et al. (2014) are over-plotted. In the upper panels, the white and blue line correspond to St = 1 (Eq. (3)), and a_frag (Eq. (9)) respectively.