CONSTRAINING THE EPOCH OF REIONIZATION FROM THE OBSERVED PROPERTIES OF THE HIGH-zUNIVERSE-Reference-Cited by-同舟云学术

CONSTRAINING THE EPOCH OF REIONIZATION FROM THE OBSERVED PROPERTIES OF THE HIGH-zUNIVERSE

Published:2016-12-29 Issue:1 Volume:834 Page:49
ISSN:1538-4357
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

Salvador-Solé Eduard,Manrique Alberto^ORCID,Guzman Rafael,Espinosa José Miguel Rodríguez^ORCID,Gallego Jesús^ORCID,Herrero Artemio^ORCID,Mas-Hesse J. Miguel,Franch Antonio Marín

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://stacks.iop.org/0004-637X/834/i=1/a=49/pdf

Reference153 articles.

1. THE EVOLUTION OF THE FAINT END OF THE UV LUMINOSITY FUNCTION DURING THE PEAK EPOCH OF STAR FORMATION $(1\lt z\lt 3)$

2. ACCRETION ONTO THE FIRST STELLAR-MASS BLACK HOLES

3. New measurements of the ionizing ultraviolet background over 2 < z < 5 and implications for hydrogen reionization

4. Detection of extended He ii reionization in the temperature evolution of the intergalactic medium★

5. Evidence for Reionization at [ITAL][CLC]z[/CLC][/ITAL] ∼ 6: Detection of a Gunn-Peterson Trough in a [ITAL][CLC]z[/CLC][/ITAL] = 6.28 Quasar

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