Observations of dim galaxies lensed by foreground clusters provides a way of measuring the progression of reionization.
What can the smallest galaxies in the local Universe tell us about reionization?
An Astronomer looks at the potential contribution of globular clusters to the global UV luminosity function during reionization.
Can we detect the signature of an AGN reionization?
Simulations of cosmic dawn reionization bubbles tell us if they can be imaged by the SKA.