Modeling results for the four debris disks discussed in this study. The Q_ϕ image (the ellipse represents where the goodness of fit is estimated), best fit model, and residuals are shown from top to bottom. From left to right, the stars are HD 191089, HD 157587, HD 115600, and HD 129590 (same as in Olofsson et al. 2022b for the latter two stars). The scaling is linear and the same for each column (colorbar shown in the middle panel). The horizontal bar in the bottom panel represents 1″.