Non-merger and merger candidates from the various surveys considered in this study, separated into Silver and Gold samples. Each row shows two representative sources for each category: non-merging systems; Silver sample mergers (selected based on the f(G, M₂₀) criterion, Eq. (1)); and Gold sample mergers (satisfying both f(G, M₂₀) and A criteria, Eqs. (1) and (2)). The cutouts, in the F115W filter, show the rest-frame UV at the redshift of each galaxy. The source ID, redshift, asymmetry (A), and Gini-M₂₀ (f(G, M₂₀)) values are provided for each stamp.