Detecting reionization in the star formation histories of high-redshift galaxies

Rennan Barkana, Abraham Loeb

Research output: Contribution to journalArticlepeer-review

Abstract

The reionization of cosmic hydrogen, left over from the big bang, increased its temperature to ≳ 104 K. This photoheating resulted in an increase of the minimum mass of galaxies and hence a suppression of the cosmic star formation rate (SFR). The affected population of dwarf galaxies included the progenitors of massive galaxies that formed later. We show that a massive galaxy at a redshift z ≳ 6 should show a double-peaked star formation history marked by a clear break. This break reflects the suppression signature from reionization of the region in which the galaxy was assembled. Since massive galaxies originate in overdense regions where cosmic evolution is accelerated, their environment reionizes earlier than the rest of the universe. For a galaxy of ∼ 1012 M in stars at a redshift of z ∼ 6.5, the SFR should typically be suppressed at a redshift z ≳ 10 since the rest of the universe is known to have reionized by z ≳ 6.5. Indeed, this is inferred to be the case for HUDF-JD2, a massive galaxy which is potentially at z ∼ 6.5 but is inferred to have formed the bulk of its 3 × 10 11 M in stars at z ≳ 9.

Original languageEnglish
Pages (from-to)395-400
Number of pages6
JournalMonthly Notices of the Royal Astronomical Society
Volume371
Issue number1
DOIs
StatePublished - Sep 2006

Keywords

  • Cosmology: theory
  • Galaxies: formation
  • Galaxies: high-redshift

Fingerprint

Dive into the research topics of 'Detecting reionization in the star formation histories of high-redshift galaxies'. Together they form a unique fingerprint.

Cite this