Comparison between thermally derived asteroid diameters and occultation-based diameters, both determined in this work (Tables 4 and 5). The horizontal axis corresponds to the CITPM-derived size, while the vertical axis is the occultation-derived size. The dashed green line is for y = x. Blue points are for the pole 1 solution, while brown points are for the pole 2 solution. Relative residuals are computed as follows: 100 × (D_CITPM − D_occ)/D_occ.