Single-star rotationally-induced chemically-homogeneous low-metallicity models at the onset of core-collapse (v_infall300km/s and does not exhibit spurious spikes in the HR diagram (this last condition is vetted by eye). The resolution tests are presented in the appendix of Gottlieb, Renzo et al. 2024. Only masses and rotation rates are varied here.For each model, inside the folder `LOGS` there are several profiles when first `log_center_T>=8.95`, oxygen depletion, silicon depletion, and onset of core collapse, plus the `history.data` file for the run. Corresponding `*.mod` files are also provided to restart the runs from these evolutionary points. `output.txt` contains the terminal output for these runs.`scripts.tar.xz` contains python scripts to reproduce the figures in the paper, see also https://github.com/mathren/CHE_lGRB_progenitors. `build.sh` allows to build the manuscript, see also README at https://github.com/mathren/CHE_lGRB_progenitors.