Simulated observations of disks located in the star-forming regions listed in Table 3 for the 1 M_J planet in the dynamic case at λ = 850  μm with an integration time of 1 h. The angular resolution for each image is given on the left (it corresponds to an identical spatial resolution for all star forming regions), together with the region’s name. 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.