Combined light, odd-Z, α-, and s-process elements. Panels a–f: [Mg/Fe]–[Al/Fe], [C/Fe]–[N/Fe], [Al/Fe]–[Ce/Fe], [Si/Fe]–[Al/Fe], [N/Fe]–[Al/Fe], and [N/Fe]–[Ce/Fe] distributions for Ton 2 (black asterisks), 47 Tucanae (orange circles) from Mészáros et al. (2020), and NGC 6380 (blue inverted triangles) from Fernández-Trincado et al. (2021a). The typical uncertainties for Ton 2 members are also shown. In panels c and f, Pearson’s (P: first row of the annotation) and Spearman’s (S: second row) coefficients (first entry) and p-values (second entry) are indicated for Ton 2 (black), NGC 6380 (blue), and 47 Tucanae (orange). As in Fig. 4, the abundance ratios shown here were determined by adopting photometric atmospheric parameters.