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

本数据集包含经降采样处理的数据，以及基于太阳金属丰度下中等超爱丁顿吸积与保守质量转移模型计算得到的CO-HMS_RLO与CO-HeMS网格对应的训练分类与插值模型。本数据集的相关说明详见Xing等人（2024）的研究。其分辨率与恒星、双星物理假设沿用Fragos等人2023年的工作，但本数据集经重新后处理，以适配POSYDON代码v2.0.0-pre1发布版（详见Andrews等人2024年的研究）。

若使用本数据集，请引用以下文献：
Xing等人（2024），预印本arXiv:2407.00200
Fragos等人（2023），《天体物理学杂志增刊系列》，第264卷第2期，文章编号45，共46页
Andrews等人（2024），预印本arXiv:2411.02376