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  4. Evolution of the observed Ly alpha luminosity function from z=6.5 to z=7.7: evidence for the epoch of reionization?
 
research article

Evolution of the observed Ly alpha luminosity function from z=6.5 to z=7.7: evidence for the epoch of reionization?

Clement, B.
•
Cuby, J.-G.
•
Courbin, F.  
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2012
Astronomy & Astrophysics

Aims. Ly alpha emitters (LAEs) can be detected out to very high redshifts during the epoch of reionization. The evolution of the LAE luminosity function with redshift is a direct probe of the Ly alpha transmission of the intergalactic medium (IGM), and therefore of the IGM neutral-hydrogen fraction. Measuring the Ly alpha luminosity function (LF) of Lya emitters at redshift z = 7.7 therefore allows us to constrain the ionizing state of the Universe at this redshift.

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Type
research article
DOI
10.1051/0004-6361/201117312
Web of Science ID

WOS:000300614100066

Author(s)
Clement, B.
Cuby, J.-G.
Courbin, F.  
Fontana, A.
Freudling, W.
Fynbo, J.
Gallego, J.
Hibon, P.
Kneib, J.-P.  
Le Fevre, O.
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Date Issued

2012

Published in
Astronomy & Astrophysics
Volume

538

Start page

A66

Subjects

methods: observational

•

early Universe

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galaxies: high-redshift

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techniques: image processing

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galaxies: luminosity function

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mass function

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dark ages

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reionization

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first stars

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Lyman-Break Galaxies

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Origins Deep Survey

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Goods-South Field

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J-Band Search

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Redshift 6

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Cosmic Variance

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1St Galaxies

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Emitters

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Emission

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Z-Similar-To-9

Editorial or Peer reviewed

REVIEWED

Written at

EPFL

EPFL units
LASTRO  
Available on Infoscience
April 5, 2012
Use this identifier to reference this record
https://infoscience.epfl.ch/handle/20.500.14299/79230
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