Relation between O32 and EW([OIII]λ5007) (top panel) and Σ_SFR (bottom panel). We include lower limits due to the non-detection of [OII]. In green symbols, the sample of EELGs with NIRSpec spectra, while in magenta symbols, the control sample with NIRSpec spectra. The vertical dashed line is the separation between weak and strong LyC leaker according to Flury et al. (2022). On the top panel, black squares are a comparison sample at z = 1.3 − 2.4 (Tang et al. 2019), and the blue dashed-dotted line is the relation found in Boyett et al. (2024) for a sample of galaxies at z = 3 − 9.5.