Constraints on the early Universe star formation efficiency from galaxy clustering and halo modeling of Hα and [O iii] emitters

This is a repository for all the measurements and results related to the Shuntov et al. 2025 paper -- "Constraints on the early Universe star formation efficiency from galaxy clustering and halo modeling of Halpha and [OIII] emitters" https://arxiv.org/abs/2503.14280 The data is stored in ecsv tables and should be self-describing. The jupyter notebook HowTo.ipynb (and the pdf document) shows examples of how to read the data and make plots.