Variation of the low-mass end of the stellar initial mass function with redshift and metallicity (dataset)

This is the dataset that was used to produce a paper published in the Monthly Notices of the Royal Astronomical Society (MNRAS): Bate (2025, submitted Sept 2024). It contains output from each of the twenty SPH simulations. It also includes data produced during the analysis of the calculations to produce the figures appearing in the paper and the Python scripts used to generate the figures. To view the paper itself, follow the associated DOI.