The same as Fig. 3, but for the MASSIV source 910274060 (major merger). The outer contour marks the 1.20 ADU (3σ_sky) isophote, while brighter isophotes increase in 1.00 ADU (2.5σ_sky) steps. The grey dot in the central figure marks the centre of the system given by the kinematical model, while the red/blue dot marks the photometric centre of the principal/companion galaxy given by the two-component model of the source. The long bars mark the position angle of the previous models. The short bar marks the photometric position angle given by the one-component model of the source. (A colour version of this plot is available at the electronic edition.)