Yields of 3D magnetorotational supernova models in Zha et al. 2024

These tables contain the nucleosynthetic yields from magnetorotational supernovae calculated by Zha, Mueller, Powell (2024), arXiv: 2403.02072. The name of the tables indicates that the models has an initial progenitor mass of 39 solar masses. B0, B10, B12 imply the initial magnetic-field strengths of 0, 10^10 and 10^12 gauss with detailed field configuration given by Equation (1) of the accompanying paper. Each table has three columns, which displace the atomic number (1st column), mass number (2nd column) and absolute mass in the unit of a solar mass (3rd column), corresponding to each isotope in the rows.