Notes. Summary of the initial conditions for the different sets of simulations. The first and second columns are Mi and Rh which are the initial mass and half-mass radius of the stellar system, respectively. The third column is the number of stars. The fourth column MBH is the black hole mass. The fifth is the time of the simulation. The sixth column shows the codes (B: bridge, SL: starlab, NB6: nbody6, NB6+: nbody6++gpu, and BF: bifrost) and the last column shows the references. The full table is available at the CDS.

References. P+99: Portegies Zwart et al. (1999), F+13: Fujii & Portegies Zwart (2013), K+15: Katz et al. (2015), M+16: Mapelli (2016), S+17: Sakurai et al. (2017), R+18: Reinoso et al. (2018), P+19: Panamarev et al. (2019), R+20: Reinoso et al. (2020), V+21: Vergara et al. (2021), V+23: Vergara et al. (2023), AS+23: Arca Sedda et al. (2023a,b,c), R+23: Rizzuto et al. (2023).