Shear weight distributions as function of measured galaxies’ properties. In the upper panel, we present the joint distribution of predicted galaxy weights by the NNs, considering the measured galaxy’s half-light radius and magnitude as variables. The lower panel illustrates the weights regarding the measured S/N Additionally, the medians of binned weights corresponding to different S/N values are depicted as blue-violet data points, accompanied by their associated 16 and 84% errors.