Data from "Short-Lived Gravitational Instability in Isolated Irradiated Discs"

The paper by Rowther et al. (2024) simulates the evolution of irradiated gravitationally unstable protoplanetary discs with live radiative transfer using Phantom (Price et al. 2018) coupled with MCFOST (Pinte et al. 2006, 2009). The codes used to perform the simulations are available at 

Phantom -- https://github.com/danieljprice/phantom

MCFOST -- https://github.com/cpinte/mcfost

The dataset contains the following data to recreate any of the figures:

Selected snapshots of the 5 simulations shown in the paper. 

Post-processed data to recreate the line-plots shown in the paper.

.fits files of the synthetic continuum images created by post-processing the simulation snapshot with MCFOST at 1.3mm.

To recreate any of the simulations in the paper, all relevant files required are in Simulations.zip.

.setup: The file used by phantomsetup to create the initial conditions of the disc.

.in: The file used by phantom to perform the simulation.

.para: A file containing the parameters used by MCFOST to perform the Radiative Transfer calculations.

The files for the 0.1 Solar mass disc can be identified by the prefix Md0p1. Similarly, the prefix Md0p25 identifies the files for 0.25 Solar mass disc.

The data to recreate any of the figures in the paper are found in Figure_*.zip.

The binary code snapshots (Md0p1_01400, Md0p25_00300 etc.) containing the raw data (particle positions, velocities, thermal energy etc.) can be visualised by Splash (Price 2007) or Sarracen (Harris & Tricco 2023). The latter was used to create the figures in the paper.

Rowther等人（2024）的研究通过将Phantom（Price等，2018）与MCFOST（Pinte等，2006、2009）耦合，并结合实时辐射传输模拟，实现了受辐照的引力不稳定原行星盘的演化模拟。
本研究使用的模拟代码可通过以下链接获取：
Phantom：https://github.com/danieljprice/phantom
MCFOST：https://github.com/cpinte/mcfost

本数据集包含可复现论文中任意图表所需的以下数据：
1. 论文中展示的5组模拟的选定快照；
2. 可复现论文中折线图的后处理数据；
3. 通过MCFOST对模拟快照进行后处理得到的1.3mm波段合成连续谱图像的.fits文件。

若要复现论文中的任意模拟，所需的全部相关文件均收录于Simulations.zip压缩包中，其中：
.setup文件：用于phantomsetup生成原行星盘的初始条件；
.in文件：用于phantom执行模拟计算；
.para文件：包含MCFOST进行辐射传输计算所需的全部参数。
以Md0p1为前缀的文件对应0.1倍太阳质量的原行星盘，同理，以Md0p25为前缀的文件对应0.25倍太阳质量的原行星盘。

可复现论文中任意图表的数据均收录于Figure_*.zip压缩包中。
二进制代码快照（如Md0p1_01400、Md0p25_00300等）包含原始模拟数据（粒子位置、速度、热能等），可通过Splash（Price，2007）或Sarracen（Harris & Tricco，2023）进行可视化处理，本论文的图表即通过后者生成。