Fraction of outflows in AGN as a function of environmental parameters. Left panel: outflows as a function of the normalized distance to the central galaxy of the group, r_cen/r₁₈₀, for AGN satellites. Right panel: outflows as a function of the projected surface density to the nearest 5th neighbour, δ₅, for all the AGNs in our sample. In both cases, we divided the sample by lower and higher mass. The heights of the boxes denote the 1σ errors associated with the fractions. Bins were defined to include at least 40 (left) and 100 (right) galaxies, respectively.