Re-postprocessed POSYDON v1.0 dataset, assuming super-Eddington accretion, compatible with code release v2.0.0-pre1
Re-postprocessed POSYDON v1.0 dataset, assuming super-Eddington accretion, compatible with code release v2.0.0-pre1
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 Xing et al. (2024). The resolution and stellar and binary physics assumptions follow Fragos et al. 2023, but the dataset is re-postprocessed to be compatible with POSYDON code release v2.0.0-pre1 (see Andrews et al. 2024). If you use this dataset, please cite the following papers: Xing et al. (2024), eprint arXiv:2407.00200Fragos et al. (2023), The Astrophysical Journal Supplement Series, Volume 264, Issue 2, id.45, 46 pp.Andrews et al. (2024), eprint arXiv:2411.02376
- University of Geneva Switzerland
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