These are the results from: "Polluting the pair-instability mass gap for binary black holes through super-Eddington accretion in isolated binaries" Authors: L.A.C. van Son, S. E. de Mink, F. S. Broekgaarden, M. Renzo, S. Justham, E. Laplace, J. Moran-Fraile, D. D. Hendriks, and R. Farmer ADS: https://ui.adsabs.harvard.edu/abs/2020arXiv200405187V/abstract arXiv: https://arxiv.org/abs/2004.05187 If you use (part of) these results in a scientific publication, we would greatly appreciate it if you would cite the source paper. This work uses COMPAS to compute binary population properties (https://github.com/TeamCOMPAS/COMPAS/tree/master/docs). ***************************** For each of our 4 model variations (0. Fiducial, 1. Stable accretion, 2. Common envelope accretion and 3. Combined) we provide 2 files: 1.) pythonSubmit.py file describing the initial conditions that were used to run the simulations 2.) COMPASOutput.h5 file, which contains the following datasets resulting from our simulations : ['systems', 'doubleCompactObjects', 'commonEnvelopes', ] Detailed descriptions of these groups can be found in the accompanying README file.