Journal Article

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

Andrea Morandi and Rennan Barkana

in Monthly Notices of the Royal Astronomical Society

Published on behalf of The Royal Astronomical Society

Volume 424, issue 4, pages 2551-2561
Published in print August 2012 | ISSN: 0035-8711
Published online August 2012 | e-ISSN: 1365-2966 | DOI: http://dx.doi.org/10.1111/j.1365-2966.2012.21240.x
Studying cosmic reionization with observations of the global 21-cm signal

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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.

Keywords: galaxies: formation; galaxies: high-redshift; cosmology: theory

Journal Article.  8327 words.  Illustrated.

Subjects: Astronomy and Astrophysics

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