Reproduction package for: 'Exploring Waveform Variations among Neutron Star Ray-tracing Codes for Complex Emission Geometries'

Data files, python scripts and notebooks to reproduce the code output comparisons performed in "Exploring Waveform Variations among Neutron Star Ray-tracing Codes for Complex Emission Geometries" by Choudhury et al. (2024; ApJ 975 202, arXiv.2406.07285). Please refer to the README for detailed information. N.B. The neutral hydrogen column density (${\rm N}_{\rm H}$) value is mentioned in the paper to be $0.2 \times 10^{20} {\rm cm}^{-2}$, whereas all the analyses in the paper, as reflected in this Zenodo package, actually uses ${\rm N}_{\rm H} = 2 \times 10^{20} {\rm cm}^{-2}$.本数据集包含可复现Choudhury等人2024年发表于《天体物理学杂志（Astrophysical Journal，ApJ）》975卷202期、预印本编号arXiv:2406.07285的论文《复杂发射几何下中子星光线追踪代码间的波形差异探究》中代码输出对比实验的数据文件、Python脚本及Jupyter笔记本。 详细信息请参阅自述文件（README）。 注意：中性氢柱密度（neutral hydrogen column density，$ m N_H$）在论文中被标注为$0.2 imes10^{20} mathrm{cm}^{-2}$，但本Zenodo数据包所复现的论文所有分析实际采用的$ m N_H$值为$2 imes10^{20} mathrm{cm}^{-2}$。