Numerical simulations of black hole-neutron star mergers with equal and near-equal mass ratios - Waveforms

The numerical gravitational waveforms for the binary configurations simulated in the paper "Numerical simulations of black hole-neutron star mergers with equal and near-equal mass ratios." The waveforms are produced using the NR code BAM, packaged in SXS 2019/NRAR format (cf. Appendix A.3 of Boyle:2019kee), grouped by resolution, and corrected to the drift of the center of mass (CoM files). Ivan Markin and Tim Dietrich gratefully acknowledge support from the Deutsche Forschungsgemeinschaft (DFG) under the project 504148597 (DI 2553/7) and the computing time granted by the Resource Allocation Board and provided on the supercomputer Emmy/Grete at NHR-Nord@Göttingen as part of the NHR infrastructure. The calculations for this research were conducted with computing resources under the project bbp00049. Tim Dietrich acknowledges funding from the European Union (ERC, SMArt, 101076369). Views and opinions expressed are those of the authors only and do not necessarily reflect those of the European Union or the European Research Council. Neither the European Union nor the granting authority can be held responsible for them.