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Fig. C.1

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Top: cumulative distribution in the apparent IAB magnitude of the total MASSIV sample (green line), the close pair sample (red line) and the total MASSIV sample with IAB ≤ 23.9 (blue line). Middle: the same than before, but the red line shows the distribution of the major merger sample. Bottom: Kolmogorov-Smirnov estimator D of the total MASSIV sample distribution against the close pair (blue solid line) and the major merger (red dashed line) distributions. We computed D for those galaxies brighter than a given IAB magnitude. The solid (dashed) horizontal line marks the minimum in the D distribution for close pairs (major mergers). The vertical solid line marks the IAB magnitude at the minimum value of D, IAB,comp = 23.9.

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