Synthetic radiative transfer images created from RADMC-3D. Each column shows the disk at a particular observing wavelength, while each row shows the disk at a particular point in the binary orbit. From top to bottom, the images are shown at: binary pericenter, during disk plane crossing, mid-orbit, the point of greatest horizontal displacement of the binary, and binary apocenter. From left to right, observing wavelengths are 1.65 μm (H-band), 800 μm, and 1.3 mm (ALMA Band 7).