A Flat Photoionization Rate at 2 ≤ z ≤ 4.2: Evidence for a Stellar-Dominated UV Background and against a Decline of Cosmic Star Formation beyond z ~ 3

  • Faucher-Giguère C
  • Lidz A
  • Hernquist L
  • et al.
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Abstract

We investigate the implications of our measurement of the Lyα forest opacity at redshifts 2 ~3. Our measurement argues against a star formation rate density declining beyond z~3, in contrast to existing state-of-the-art determinations of the cosmic star formation history from direct galaxy counts. Stellar emission from galaxies therefore likely reionized the universe.

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Faucher-Giguère, C.-A., Lidz, A., Hernquist, L., & Zaldarriaga, M. (2008). A Flat Photoionization Rate at 2 ≤ z ≤ 4.2: Evidence for a Stellar-Dominated UV Background and against a Decline of Cosmic Star Formation beyond z ~ 3. The Astrophysical Journal, 682(1), L9–L12. https://doi.org/10.1086/590409

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