Supplementary material for "A Toomre-motivated structural acceleration proxy in disc galaxies"

This record contains the supplementary and reproducibility material for the manuscript “A Toomre-motivated structural acceleration proxy in disc galaxies” by Alim ul Haq Khan. The material includes simulation notebooks, generated numerical tables, figure-generation scripts, supplementary figures, and supporting files used to reproduce the Monte Carlo experiments and diagnostic plots discussed in the manuscript. The study examines a Toomre-motivated structural acceleration proxy, gcrit = σV/R, and tests whether its baryonic-mass dependence cancels under empirical disc-galaxy scaling relations. This Zenodo record is provided as supplementary/reproducibility material and is not a separate peer-reviewed publication.本数据集记录包含Alim ul Haq Khan所撰论文《基于图姆尔（Toomre）理论的盘状星系结构加速度代理指标》的补充与可复现材料。 该材料涵盖模拟代码笔记、已生成的数值表格、绘图脚本、补充图表及辅助文件，用于复现论文中所述的蒙特卡洛（Monte Carlo）实验与诊断绘图。 本研究针对基于图姆尔理论的结构加速度代理指标gcrit = σV/R展开分析，检验其重子质量依赖性是否在经验盘状星系标度关系下得以抵消。本Zenodo数据集仅作为补充与可复现材料提供，并非独立的同行评议出版物。