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Title:
The Volume Fraction of Ionized Intergalactic Gas at Redshift z=6.5
Authors:
Malhotra, Sangeeta; Rhoads, James E.
Affiliation:
AA(School of Earth and Space Exploration, Arizona State University, P.O. Box 871404, Tempe, AZ 85287-1404 , ), AB(School of Earth and Space Exploration, Arizona State University, P.O. Box 871404, Tempe, AZ 85287-1404 , )
Publication:
The Astrophysical Journal, Volume 647, Issue 2, pp. L95-L98. (ApJL Homepage)
Publication Date:
08/2006
Origin:
UCP
ApJ Keywords:
Galaxies: High-Redshift, Galaxies: Intergalactic Medium
DOI:
10.1086/506983
Bibliographic Code:
2006ApJ...647L..95M

Abstract

The observed number density of Lyα sources implies a minimum volume of the intergalactic medium that must be ionized, in order to allow the Lyα photons to escape attenuation. We estimate this volume by assigning to each Lyα emitter the minimum ionized bubble that would allow half its Lyα photons to escape. This implies a lower limit to the ionized gas volume fraction of 20%-50% at z=6.5. This is a lower limit in two ways: First, we conservatively assume that the Lyα sources seen (at a relatively bright flux limit) are the only ones present, and second, we assume the smallest ionized bubble volume that will allow the photons to escape. This limit is completely independent of what ionizing photon sources produced the bubbles. Deeper Lyα surveys are possible with present technology and can strengthen these limits by detecting a higher density of Lyα galaxies.
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