Data behind Heather et al. (2026), "Extreme Values of Black Hole to Stellar Mass Ratio for High-Redshift Galaxies"

This deposit contains the high-level numerical data underlying select figures and tables in Heather, Chantavat, Chongchitnan & Silk (2026) [arXiv:2604.02568]. The paper applies extreme-value statistics (EVS) to predict extreme black-hole-to-stellar-mass ratios (M_BH/M*) for galaxies at redshift 3.5 < z < 8.5, using two independent pipelines described in Sections 4 and 5 of the paper. For more information, see ReadMe.md.