Notes. Integrations were performed using the fourth-order Hermite predictor corrector for 10⁴ N-body time units with a time-step parameter of η = 0.01, and with outputs every 0.1 time unit. The first column identifies the interaction, followed by the braid’s total energy in N-body units [mass⋅(length/time)²], and the period of one complete orbit. The Lyapunov timescale (fourth column) was calculated by introducing a small perturbation (of 10⁻⁵) in the x-coordinate of the first particle. The fifth column gives t_stable, the integration time over which we could determine that the system remained stable with a maximum integration time of t_stable = 10⁴. Note that we classify $I.A{.}_{68}^{i.c.}(0.5)$ as marginally stable, discussed in Sect. 4.1. The following column gives the number of experiments calculated while varying m_in, the impact parameter and relative encounter velocity. The last 4 columns give the fraction of interaction that leads to the various outcomes (marginalized over v_in, m_in, and d_in), binary-single-single (BSS), four single stars (4S), binary-binary (BB), and triple-single (TS).