Datasets for "Pulsational pair-instability supernovae in gravitational-wave and electromagnetic transients" from Hendriks et al 2023.

Data related to the paper "Pulsational pair-instability supernovae in gravitational-wave and electromagnetic transients" by Hendriks et al 2023 https://doi.org/10.1093/mnras/stad2857. `EVENTS_V2.2.2_SEMI_HIGH_RES*.tar.gz: main PPISN prescription variation simulation results for the GW mergers. These contain configurations for the populations and the convolved merger results which in turn contain merger rates, merger properties and events that preceded the mergers (RLOF episodes, SNe). These results are used in figures 2, 3, 6, and 7. Figure 8 uses the SFR used in one of these simulations. `EVENTS_V2.2.2_MID_RES*.tar.gz`: PPISNe prescription variation results for the transient rate evolution. These contain configurations for the populations and the convolved merger results which in turn contain merger rates, merger properties and events that preceded the mergers (RLOF episodes, SNe). These results are used in figure 4. `grid_single_mass_metallicity_data.tar.gz`: data containing single-star remnant-mass data as a function of initial mass vs. final mass for our fiducial model and three variations: Farmer 2019 PPISN prescription, M_extra_ppisn_ML=10 Msun (i.e. where 10 solarmass of additional mass loss occur for each PPISN), M_co_shift_ppisn=-5 Msun (i.e. the CO core mass range that undergoes PPISN is shifted to lower masses by 5 solarmass). This data is used in figure 5. `schematic_overview_data.tar.gz`: data containing single-star remnant-mass data as a function of pre-SN core mass for our fiducial models and several variations: Farmer 2019 PPISN prescription, M_extra_ppisn_ML = 5 Msun, M_co_shift_ppisn=-5 Msun, M_co_shift_ppisn=+5 Msun. This data is used in figure 1. `paper_ppisne_scripts-main.tar.gz`: git-repository that contains the routines to generate the figures. The readme in this script should contain enough information, but relevant to the data here: the user needs to store the files contained in this zenodo repository in a directory that they point to at with an environment variable called `paper_PPISNe_Hendriks2023_data_dir`. These scripts are also hosted on https://gitlab.com/dhendriks/paper_ppisne_scripts本数据集关联Hendriks等人2023年发表的论文《引力波与电磁暂现源中的脉动对不稳定性超新星（Pulsational pair-instability supernovae，PPISN）》，论文DOI为10.1093/mnras/stad2857。 `EVENTS_V2.2.2_SEMI_HIGH_RES*.tar.gz`：针对引力波并合事件的核心PPISN处方变体模拟结果。该数据集包含种群配置与卷积后的并合结果，其中并合结果涵盖并合率、并合特性以及并合前的相关事件（洛希瓣溢流（Roche Lobe Overflow，RLOF）事件、超新星）。本数据集用于制作图2、图3、图6与图7。图8则采用了本数据集其中一项模拟中使用的恒星形成率（Star Formation Rate，SFR）。 `EVENTS_V2.2.2_MID_RES*.tar.gz`：针对暂现源率演化的PPISN处方变体结果。该数据集包含种群配置与卷积后的并合结果，其中并合结果涵盖并合率、并合特性以及并合前的相关事件（RLOF事件、超新星）。本数据集用于制作图4。 `grid_single_mass_metallicity_data.tar.gz`：包含单星遗迹质量数据的数据集，数据以初始质量与最终质量的函数关系形式呈现，对应本研究的基准模型与三类变体：Farmer 2019年提出的PPISN处方、`M_extra_ppisn_ML=10 Msun`（即每一次PPISN事件额外发生10倍太阳质量的质量损失）、`M_co_shift_ppisn=-5 Msun`（即发生PPISN的碳氧核心质量范围向更低质量方向偏移5倍太阳质量）。本数据集用于制作图5。 `schematic_overview_data.tar.gz`：包含单星遗迹质量数据的数据集，数据以超新星前核心质量的函数关系形式呈现，对应本研究的基准模型与四类变体：Farmer 2019年提出的PPISN处方、`M_extra_ppisn_ML = 5 Msun`、`M_co_shift_ppisn=-5 Msun`以及`M_co_shift_ppisn=+5 Msun`。本数据集用于制作图1。 `paper_ppisne_scripts-main.tar.gz`：包含绘图相关程序的Git代码仓库。该脚本自带的自述文件已提供足够说明信息，针对本数据集的使用要求为：用户需将本Zenodo仓库中的文件存储至指定目录，并通过名为`paper_PPISNe_Hendriks2023_data_dir`的环境变量指向该目录。本脚本同样托管于https://gitlab.com/dhendriks/paper_ppisne_scripts