Simulated observations for the 1 M_J planet in the dynamic case at λ = 850  μm. From left to right: integration time of 10 min, 30 min, 1 h, 2 h, 4 h and 8 h. From top to bottom: angular resolution of 0.05″, 0.10″, 0.15″, 0.30″ and 0.50″ (the ALMA configuration is adapted to match the angular resolution for each wavelength). The scale on each image is in arcseconds, with the beam size represented at its bottom left corner, and the colorbar gives the flux in mJy/beam. (Note that the flux scale changes in each row, due to the different beam size.)