Outcomes of the dynamically unstable phase for the full population of triples that become dynamically unstable during their evolution. Pie-charts represent the N-body simulations with stellar evolution for model OBin. The histograms show the outcomes for all models where different colours represent the different dynamical methods (Sect. 3.2). Solid, dashed, and dotted line styles represent the models for the initial population of triples OBin, T14 and E09, respectively. The results for each model are normalised to unity.