Studying cosmic reionization with observations of the global 21-cm signal

Andrea Morandi, Rennan Barkana

Research output: Contribution to journalArticlepeer-review

Abstract

We explore the ability of observations of the global brightness temperature of the 21-cm signal to constrain the reionization history and the properties of the ionizing sources. In order to describe the reionization signal, we employ either a commonly used toy model or a more realistic structure formation model that parametrizes the properties of the ionizing sources. If the structure formation model captures the actual evolution of the reionization signal, then detecting the signal is somewhat easier than it would be for the toy model; using the toy model in this case also leads to systematic errors in reconstructing the reionization history, though a sufficiently sensitive experiment should be able to distinguish between the two models. We show that under optimistic assumptions regarding systematic noise and foreground removal, 1-year observations of the global 21-cm spectrum should be able to detect a wide range of realistic models and measure the main features of the reionization history while constraining the key properties of the ionizing sources.

Original languageEnglish
Pages (from-to)2551-2561
Number of pages11
JournalMonthly Notices of the Royal Astronomical Society
Volume424
Issue number4
DOIs
StatePublished - 21 Aug 2012

Keywords

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

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