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Cited by 336

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Luminosity Functions of Lyα Emitters at Redshifts z = 6.5 and z = 5.7: Evidence against Reionization at z ≤ 6.5

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Malhotra, Sangeeta, Rhoads, James E.·2004·The Astrophysical Journal

Abstract

The visibility of Lyα emission from galaxies should be suppressed substantially by a neutral intergalactic medium before reionization. Even after taking into account a local H II region produced by the galaxy and a velocity offset of Lyα, a factor of 3 attenuation in the line is unavoidable. We rule out such a suppression by comparing line luminosity functions of Lyα emitters at z = 6.5 and 5.7. The luminosity functions at z = 5.7 and z = 6.5 were constructed using published surveys over a range of depths and volumes. They constrain both characteristic luminosity L * and density ϕ * . The luminosity functions at the two redshifts are statistically consistent with one another, and only one survey lies substantially off the luminosity function. We conclude that reionization was largely complete at z ≈ 6.5.

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Metadata

Authors
Malhotra, S., & Rhoads, J. E.
Venue
The Astrophysical Journal
Published
2004-11-11
Volume
617
Issue
1
Pages
L5-L8
ISSN
  • 0004-637X (ISSN-L)
  • 1538-4357
OpenAlex
W2072053764
Cited by
336
References
2
FWCI
15.16
Type
journal article
Language
en
Open access
bronze

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CoChat. (2026). Citation check: Luminosity Functions of Lyα Emitters at Redshifts z = 6.5 and z = 5.7: Evidence against Reionization at z ≤ 6.5. https://app.cochat.ai/papers/10.1086/427182
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Malhotra, S., & Rhoads, J. E. (2004). Luminosity Functions of Lyα Emitters at Redshifts z = 6.5 and z = 5.7: Evidence against Reionization at z ≤ 6.5. The Astrophysical Journal. https://doi.org/10.1086/427182

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Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).

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