Normalized intensity as a function of orbital distance at 1.5 Myr, comparing the uncolvolved intensity with the ones convolved with three different beams of 0.02′′ and 0.04′′ at 140 pc (2.8 and 5.6 AU), and 0.34″ at 232 pc (100 AU). The gray dashed lines show the evaporation fronts that mainly cause the spikes in the intensity. The examples with a giant correspond to the standard set of parameters (Fig. 1), while the example without a giant corresponds to a low-mass disk (top left plot in Fig. 2).