Gamma-Ray Bursts Reveal the History and Faint Contributors of Cosmic Reionization

Star-forming galaxies are generally believed to be the main drivers of cosmic reionization. However, the relative contributions of bright and faint galaxies to this process remain unclear. As the most luminous transient phenomena in the universe, long gamma-ray bursts (LGRBs) provide a unique opportunity to probe star formation occurring in both detectable and undetectable galaxies. In this Letter, we present new estimates of the cosmic star formation rate density (SFRD) at 4 < z < 10 using Swift LGRBs detected over the past two decades, by considering LGRBs as unbiased tracers of total star formation at high redshifts. Crucially, we find that the new LGRB-inferred SFRD can naturally explain current measurements of hydrogen reionization without invoking extreme ionizing photon production efficiencies or escape fractions from galaxies. Using these LGRB-inferred SFRD values, we further investigate the faintest magnitude limits of high-redshift galaxies, finding a redshift evolution of the limiting magnitudes from (Formula presented) Mlim∼−14 to −15 at z ∼ 6, to (Formula presented) Mlim∼−10 to −11 at z ∼ 10. This result provides one independent piece of evidence for the presence of a large population of faint galaxies at redshifts z ≳ 6, as an important complement to our understanding of the ionizing photon budget in the early universe.