Same as Figures 11 and 12, but for the ﹩{\dot{M}}_{{\rm{in}}}=1{0}^{-6}\,{M}_{\odot }\,{{\rm{yr}}}^{-1}﹩ model. The residuals are dominated by the eccentric disk and disk warp, which produce prominent arc-like structures and significantly distort the disk’s kinematic position angle.
