Description
1- Prospects for constraining Reionization History with the Ly-alpha Line: Transmission Statistics, Clustering, or other methods.
2- What are the most promising techniques for constraining Lyman-continuum escape from high-z galaxies?
3- Calibrating the relationship between galaxy properties and ionizing photon production.
4- Reaching for zero metallicity: what will we learn from JWST about Population III stars, the production of metals in galaxies, and the enrichment of the IGM.
