Notes. The number of calculated close encounters (N_enc) per 1000 simulated orbits is indicated for each star-subgroup pair, along with the mean minimum separation (${\overline{s}}_{\text{min}}$), how far in the past the encounter occurred ($t({\overline{s}}_{\text{min}})$), the peculiar velocity of the candidates with respect to the corresponding subgroups (v_pec,3D) as well as the ratio between the number of true close encounters and the number of random pairings (P_enc/P_rnd). For each star-subgroup pair, a flag indicates which ejection scenario is the likeliest based on the difference between the subgroup’s age and the time that has passed since the ejection; if the difference is below 3 Myr, it likely was ejected dynamically (DES) and if the difference is 3–4 Myr, it was ejected by either DES or BSS. Otherwise, the ejection was likely caused by the binary supernova scenario (BSS). Note that initially, in order to identify the most promising runaway candidates (i.e., those listed here), 1000 traceback simulations were run per star-subgroup pair. For this selection of candidates, the traceback simulations were repeated, but this time with 300 000 runs for each star-subgroup pair; the column N_enc now lists the number of calculated encounters from these repeated traceback runs scaled down to 1000 simulations in order to maintain comparability with Fig. 1 and our reasoning described in Sect. 2.4. Additionally, for each star, the literature was checked in order to determine whether it was previously known as a runaway star, where Tetzlaff et al. (2011, abbreviated as T11), Hoogerwerf et al. (2001, H01), Mdzinarishvili (2004, which did not include any of the stars presented here), Mdzinarishvili & Chargeishvili (2005, which also did not include any of these stars), Carretero-Castrillo et al. (2023, which did not include the stars presented here, either), and Maíz Apellániz et al. (2018, MA18) were used as references. We note that γ Gru (T11), γ Crv (T11), and ζ Oph (T11, H01, MA18) are indeed known runaway stars or candidates.