Cosmic reionization and early star-forming galaxies: A joint analysis of new constraints from planck and the Hubble Space Telescope

Brant E. Robertson, Richard S. Ellis, Steven R. Furlanetto, James S. Dunlop

Research output: Contribution to journalArticle

329 Scopus citations

Abstract

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 z ≃ 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 τ = 0.066 ± 0.012 recently reported by the Planck collaboration and the evolving neutrality of the intergalactic medium with a reionization history within 6 ≲ z ≲ 10, thereby reducing the requirement for a significant population of very high redshift (z 蠑 10) galaxies. Our analysis strengthens the conclusion that starforming 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.

Original languageEnglish (US)
Article numberL19
JournalAstrophysical Journal Letters
Volume802
Issue number2
DOIs
StatePublished - Apr 1 2015

    Fingerprint

Keywords

  • Galaxies: high-redshift

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

Cite this