Abundances and nuclear heating rates

In the following, we provide the abundances (at 100 days) and the nuclear heating rates for specified ejecta properties

If you make use of the provided data, please make sure to read and cite the following paper:

• Heavy elements and electromagnetic transients from neutron star mergers, S. Rosswog & O. Korobkin
  arXiv:2208.14026 (2022)