Rms dimensions of the automatically detected (p ≤ 0.05) structures in circular areas around the central host galaxy. These dimensions were calculated via the small angle approximation assuming all dwarfs are at the distance of the targeted host galaxy. Shown are the structure length (a), height (b), and axis ratio (c). Measured values of several well-studied planes are over plotted for comparison purposes. References for these are: Pawlowski et al. (2013) (VPOS, GPoA), Müller et al. (2018a) (CASP), Tully et al. (2015), Müller et al. (2016) (CenA_P1, CenA_P2).