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Fig. D.1.

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Results of the analysis of HD135344B dust substructures performed with DBNets2.0 (Ruzza et al. 2025). The plot is constructed sampling 5 ⋅ 105 points from the inferred posterior distribution for the four target disc and planet properties. Axis limits correspond to the region of the parameter space where DBNets2.0 was trained. The solid vertical lines in the histograms mark the medians of the respective distributions while the dashed lines mark the 16th and 84th percentiles when these are within the plotted intervals. The deprojected ALMA Band 6 dust continuum observation (ADS/JAO.ALMA#2018.1.01066.S, Casassus et al. 2021) used for this analysis is shown in the upper right corner.

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