Reionization with star-forming galaxies: insights from the Low-z Lyman Continuum Survey

Abstract

The fraction of ionizing photons escaping from galaxies, $f_{esc}$, is at the same time a crucial parameter in modelling reionization and a very poorly known quantity, especially at high redshift. Recent observations are starting to constrain the values of $f_{esc}$ in low-z star-forming galaxies, but the validity of this comparison remains to be verified. Applying at high-z the empirical relation between $f_{esc}$ and the UV slope trends derived from the Low-z Lyman Continuum Survey, we use the DELPHI semi-analytical galaxy formation model to estimate the global ionizing emissivity of high-z galaxies, which we use to compute the resulting reionization history. We find that both the global ionizing emissivity and reionization history match the observational constraints. Assuming that the low-z correlations hold during the epoch of reionization, we find that galaxies with $-16\lesssim M_{UV}\lesssim -13.5$ are the main drivers of reionization. We derive a population-averaged $⟨f_{esc}⟩\simeq 8\%,10\%,20\%$ at z=4.5, 6, 8.

5+1 page, 3 figures, submitted to A&A