Noise free, smoothed SZ images of the plane-of-sky (upper six panels) and line-of-sight geometries (lower six panels), corresponding to the upper and lower panels of Fig. 15. First and third rows: images for an AtLAST-like resolution at 150 GHz, second and third rows: images for a CMB-S4-like resolution. The columns correspond to the representative redshifts of z = [0.057, 0.3, 0.87], chosen to correspond to the mergers in e.g., A3667, the Bullet Cluster, and El Gordo. We note that features at levels |y_kSZ|< 10⁻⁶ will likely be masked by the primary CMB on arcminute scales.