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. Good progress has been made in charting the end of reionization through spectroscopic studies of 6–8 QSOs, gamma-ray bursts, and galaxies expected to host Lyα emission. However, the most stringent constraints on its duration have come from the integrated optical depth, τ, of Thomson scattering to the cosmic microwave background. Using the latest data on the abundance and luminosity distribution of distant galaxies from Hubble Space Telescope imaging, we simultaneously match the reduced value recently reported by the Planck collaboration and the evolving neutrality of the intergalactic medium with a reionization history within , thereby reducing the requirement for a significant population of very high redshift () galaxies. Our analysis strengthens the conclusion that star-forming galaxies dominated the reionization process and has important implications for upcoming 21 cm experiments and searches for early galaxies with the James Webb Space Telescope.
|Number of pages||5|
|Journal||Astrophysical Journal Letters|
|Publication status||Published - 1 Apr 2015|
- galaxies: high-redshift
- ULTRA-DEEP FIELD
- UV LUMINOSITY FUNCTIONS
- LYMAN BREAK GALAXIES
- SIMILAR-TO 7
- INTERGALACTIC MEDIUM
- KECK SPECTROSCOPY
- ALPHA EMISSION
- THAN 8
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- School of Physics and Astronomy - Professor of Extragalactic Astronomy and Head of School
Person: Academic: Research Active