Image and lens models for BRI0952 isolated to the velocity range in which Comp-N and Comp-SW manifest. The diamond in the first three rows shows the best-fit position of the lens. Panels from top to bottom: Row 1 shows the ALMA band-7 dirty image with contours at 3, 4, 5, 6, 8, 10, 12, 14, and 16 σ levels and the magnification value found for that bin; row 2 shows the image plane model from VISILENS with the same contour levels as row 1 and the residuals after the subtraction of the VISILENS model, contours are at -3, -2, 2, and 3 σ levels; row 4 shows the image plane model from VISILENS, and the red circle and point represent the critical and caustic lines; row 5 shows the source plane model with the black dashed ellipse showing the position of the source. All images are centered around the ALMA phase center (the (0.0, 0.0) coordinate in this case; see Table 3).