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Constraints on the Star Formation Efficiency of Galaxies During the Epoch of Reionization
Guochao Sun, Steven R. Furlanetto
Reionization is thought to have occurred in the redshift range of , which is now being probed by both deep galaxy surveys and CMB observations. Using halo abundance matc…
The 21-cm Line as a Probe of Reionization
Steven R. Furlanetto
One of the most exciting probes of the early phases of structure formation and reionization is the spin-flip line of neutral hydrogen, with a rest wavelength of 21 cm. This chapter…
Reionization Through the Lens of Percolation Theory
Steven R. Furlanetto, S. Peng Oh
The reionization of intergalactic hydrogen has received intense theoretical scrutiny over the past two decades. Here, we approach the process formally as a percolation process and…
The Distribution of Bubble Sizes During Reionization
Yin Lin, S. Peng Oh, Steven R. Furlanetto +1
A key physical quantity during reionization is the size of HII regions. Previous studies found a characteristic bubble size which increases rapidly during reionization, with appare…
Large fluctuations in the hydrogen-ionizing background and mean free path following the epoch of reionization
Frederick B. Davies, Steven R. Furlanetto
Extremely large opaque troughs in the Lyman-alpha forest have been interpreted as a sign of an extended reionization process below z~6. Such features are impossible to reproduce wi…
Cosmic Reionization and Early Star-Forming Galaxies: A Joint Analysis of New Constraints from Planck and Hubble Space Telescope
Brant E. Robertson, Richard S. Ellis, Steven R. Furlanetto +1
We discuss new constraints on the epoch of cosmic reionization and test the assumption that most of the ionizing photons responsible arose from high redshift star-forming galaxies.…