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Published April 1, 2015 | Published + Accepted Version
Journal Article Open

Cosmic Reionization and Early Star-Forming Galaxies: A Joint Analysis of New Constraints from Planck and the Hubble Space Telescope


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 ≫ 10) 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.

Additional Information

© 2015 American Astronomical Society. Received 2015 February 6; accepted 2015 March 2; published 2015 April 1. We acknowledge useful discussions with George Efstathiou and Martin Haehnelt. This work was supported by Space Telescope Science Institute under award HST-GO-12498.01 A and the National Science Foundation under grant No. 1228509. J.S.D. acknowledges the support of the European Research Council via the award of an Advanced Grant, and the contribution of the EC FP7 SPACE project ASTRODEEP (Ref. No. 312725).

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Accepted Version - 1502.02024v1.pdf

Published - Robertson_2015_ApJL_802_L19.pdf


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August 20, 2023
August 20, 2023