Re-postprocessed POSYDON v1.0 dataset, assuming super-Eddington accretion, compatible with code release v2.0.0-pre1

<p>This dataset includes the downsampled data, as well as the trained classification and interpolation models, from the CO-HMS_RLO and CO-HeMS grids calculated with moderately super-Eddington accretion and conservative mass transfer model, at solar metallicity. This dataset is described in&nbsp;<a href="https://ui.adsabs.harvard.edu/abs/2024arXiv240700200X/abstract">Xing et al. (2024)</a>. The resolution and stellar and binary physics assumptions follow &nbsp;<a href="https://ui.adsabs.harvard.edu/abs/2023ApJS..264...45F/abstract">Fragos et al. 2023</a>, but the dataset is re-postprocessed to be compatible with POSYDON code release <strong>v2.0.0-pre1</strong> (see <a href="https://ui.adsabs.harvard.edu/abs/2024arXiv241102376A/abstract">Andrews et al. 2024</a>).&nbsp;</p> <p>If you use this dataset, please cite the following papers:</p> <p><a href="https://ui.adsabs.harvard.edu/abs/2024arXiv240700200X/abstract">Xing et al. (2024), eprint arXiv:2407.00200</a><br><a href="https://ui.adsabs.harvard.edu/abs/2023ApJS..264...45F/abstract">Fragos et al. (2023), The Astrophysical Journal Supplement Series, Volume 264, Issue 2, id.45, 46 pp.</a><br><a href="https://ui.adsabs.harvard.edu/abs/2024arXiv241102376A/abstract">Andrews et al. (2024), eprint arXiv:2411.02376</a></p>