Shape models of Julia reconstructed by ADAM based on differing factors: (i) combinations of shape supports (i.e., octanoid and subdivision); (ii) treatment of the AO data (weighting images according to quality) and occultation measurements (with or without); and (iii) shape model resolution. Panels 1–6 are based on octanoid and panel 7 on subdivision shape supports. We utilized stellar occultations for the computation of the models in panels 5 and 6. The enhanced shape model resolution was used in cases 2, 4, 6, and 7. Finally, the differences between models 1 and 3 and between 2 and 4 come from different weights applied to several AO images. The model in panel 4 is the one we chose. It is based on deconvolved SPHERE data and octanoid shape support with enhanced shape model resolution.