Supporting data for "THE ORIGIN OF GIANT PLANETS IN THE GJ 1148 SYSTEM"

This is original data for the thesis "THE ORIGIN OF GIANT PLANETS IN THE GJ 1148 SYSTEM". 3rd_0.1MJUP_4RH and 3rd_0.227MJUP_SameMassToGJ1148c are data for the scattering experiments of GJ 1148 systems with a hypothetical third planet of 0.1 and 0.227 Jupiter's mass. Tidal_GJ1148b is the data set for studying the spin evolution of the GJ 1148b due to the tidal interaction with the M-dwarf star. In Rep_Anderson, we use the N-body code REBOUND and SyMBA-GR to reproduce the results in K.R. Anderson (2020).本数据集为论文《GJ 1148系统中巨行星的起源》（英文原标题：THE ORIGIN OF GIANT PLANETS IN THE GJ 1148 SYSTEM）的原始研究数据。 3rd_0.1MJUP_4RH与3rd_0.227MJUP_SameMassToGJ1148c为GJ 1148系统的散射实验数据集，分别对应引入质量为0.1倍木星质量、0.227倍木星质量的假设第三颗行星的实验场景。 Tidal_GJ1148b为研究GJ 1148b与M型矮星（M-dwarf）之间潮汐相互作用所引发的自旋演化过程的数据集。 在Rep_Anderson数据集中，我们使用N体数值模拟程序REBOUND与SyMBA-GR，复现了K.R. Anderson（2020）中的研究结果。