SPHERE observations of 2MASSJ1612 system in H band (1.6 μm) and radiative-transfer-model images created from hydrodynamic simulations. The only parameter varying between the models is the mass of the injected planet indicated in the upper left of each panel. Note that we show total intensity, including the planet thermal emission for the models, while the polarized-light image of the observation is not sensitive to planet thermal emission.