Challenging a binary neutron star merger interpretation of GW230529 - Numerical Waveforms

The numerical gravitational waveforms for the binary configurations simulated in the paper "Challenging a binary neutron star merger interpretation of GW230529" (Markin:2025oeo / arXiv:2508.08750). The waveforms are produced using the NR code BAM, packaged in SXS 2019/NRAR format (cf. Appendix A.3 of Boyle:2019kee), and are grouped by resolution. Changes in v2:* For the high resolution, waveforms corrected for center-of-mass drift were added (Woodford:2019tlo) * The higher modes were reintegrated using appropriate cutoff frequencies * The BAM-SXS sign difference for modes with negative $m$ 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.