Underlying data for the paper "Efficient black hole seed formation in low metallicity and dense stellar clusters with implications for JWST sources"

Here we provide the underlying data for the 5 extremely dense Nbody star cluster models simulated as part of the preprint: https://arxiv.org/abs/2508.14260 For each model, the following 5 files are provided (where * is the original number of particles of each model): unit_conversion.dat provide the scale to convert from Nbody units to megayears. 1. RLAGR.dat_N* Tracks the evolution of the Lagrangian radii (with the VMS/IMBH). Columns in order: time [NB], lagragian (%): 0.1, 0.3, 0.5, 1, 3, 5, 10, 20, 30, 40, 50, 60, 70, 80, 90, 95, 99, 100. 2. coll.13_N* List of collisions within the cluster. Columns in order: time [NB], ID first star, ID second star, ID first star, ID second star, ID new star, mass first star [M⊙], mass second star [M⊙], mass new star [M⊙]. 3. vms.dat_N* List of stellar evolution data for the VMS/IMBH. Columns in order: time [NB], stellar type, mass [M⊙], log(radius) [R⊙], age [Myr]