Radial profiles of the theoretical images (left panels) and simulated observations (right panels) of a 3 Myr disc with a planet of mass Mp = [1,9,15] MJupfrom upper to lower panels in the R (0.65 μm), H (1.6 μm), and 850 μm bands. Solid lines correspond to intensity (I) profiles while dashed lines correspond to polarised-intensity (PI). The vertical dotted black line indicates the radial position of the planet at 20 AU.
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