Disk population synthesis data for the article: "Large gaps and high accretion rates in photoevaporative transition disks with a dead zone"

We make available here the results of our gas evolution simulations for the article "Large gaps and high accretion rates in photoevaporative transition disks with a dead zone".

We include the result of our population synthesis study, consisting in 10 tables corresponding to 9 models including both dead zone and photoevaporation, and 1 control model including photoevaporation only. The results can be plotted using the "Plotting-PopulationSynthesisModels.ipynb" jupyter notebook.

The tables including a dead zone are named as: Macc_Rhole_Pop_AD(X)_RD(Y).txt, where (X)*1.e-4 corresponds to the turbulence in the dead zone, and (Y)*AU corresponds to the dead zone radial extent.

The tables include the following fields: Simulation ID, Time [Myr] at which the snapshot was taken, Gap size [AU] measured at the outer edge, Accretion rate log[Msun/yr], and Gas disk mass. We also include a table called "LxRc_Distribution.txt", that indicates the X-ray luminosity log[erg/s] and initial disk characteristic radius [AU] used for the corresponding Simulation ID.

We also include the gas surface density evolution of a Control simulation, with photoevaporation only (with Lx = 1.e30 erg/s), and a Dead Zone + Photoevaporation simulation (with dead zone turbulence 1.e-4, and dead zone radial extend 10 AU). These can be plotted using the "Plotting-SingleGasEvolution.ipynb" jupyter notebook.

本数据集公开发布了论文《带死区（dead zone）的光蒸发（photoevaporation）过渡盘中的大间隙与高吸积率》中气体演化模拟的相关结果。

本研究包含群体合成（population synthesis）研究的全部结果：共10张数据表，对应9个同时包含死区与光蒸发过程的模型，以及1个仅包含光蒸发过程的对照模型（control model）。所有结果可通过Jupyter Notebook文件"Plotting-PopulationSynthesisModels.ipynb"进行可视化绘制。

包含死区的数据表命名格式为：Macc_Rhole_Pop_AD(X)_RD(Y).txt，其中(X)×10^-4代表死区内的湍流强度，(Y)×天文单位（astronomical unit, AU）代表死区的径向范围。

每张数据表包含以下字段：模拟ID（Simulation ID）、快照拍摄时刻[单位：百万年（Myr）]、外边缘处测得的间隙尺寸[单位：天文单位（AU）]、吸积率对数[单位：太阳质量每年（M☉/yr）]，以及气体盘质量。此外，本数据集还包含一张名为"LxRc_Distribution.txt"的数据表，该表记录了对应模拟ID所使用的X射线光度对数[单位：尔格每秒（erg/s）]与初始盘特征半径[单位：天文单位（AU）]。

本数据集还包含两组演化模拟的气体面密度（gas surface density）数据：一组为仅含光蒸发过程的对照模拟（Lx=1×10^30 erg/s），另一组为包含死区与光蒸发的模拟（死区湍流强度为1×10^-4，死区径向范围为10天文单位（AU））。所有数据可通过Jupyter Notebook文件"Plotting-SingleGasEvolution.ipynb"进行可视化绘制。