Clustering of the absorbers around LAEs. Left panel: LAE luminosity function within |Δv|≤500 km s⁻¹ of the Mg II absorbers (orange) compared to the field control sample (red, MAGG V) and to the results for LAEs around other tracers studied in MAGG (high-column density hydrogen absorbers in green from MAGG IV, C IV, and Si IV systems in black and purple from MAGG V and quasars in blue from Fossati et al. 2021). We show the parametric (line) and nonparametric (data points) estimates for each sample. Right panel: Projected cross-correlation function for LAEs within |Δv|≤500 km s⁻¹ of the Mg II absorbers (orange) assuming γ = 1.8 (solid line) and γ = 2.2 (dotted line). The other populations explored in MAGG are shown with the same colors adopted in the left panel, while the LAEs auto-correlation function derived in MAGG V is shown in red. Vertical error bars are derived by bootstrapping the redshift of the Mg II absorbers over 1000 iterations.