[Mg/Fe] versus [Fe/H] (left) and [Si/Fe] versus [Fe/H] (right) for the globular cluster VVV CL002 (red circle) compared with the abundances of other known globular clusters indicated by green circles (Mészáros et al. 2020; Carretta et al. 2009; Dias et al. 2016; Recio-Blanco 2018; Barbuy et al. 2018, 2021; Geisler et al. 2021; Schiavon et al. 2024) and bulge field stars indicated by small dots (Abdurro’uf 2022; Queiroz et al. 2023). The globular cluster mean abundances with their respective errors are all from mid- and high-resolution optical and IR spectroscopy from the literature as compiled by Garro et al. (2023). A few representative globular clusters that show abundances similar to those of VVV-CL002 are also marked with crosses and are labelled for comparison.