Predicting the merger fraction of Lyα emitters from redshift z ∼ 3 to 7
Author:
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/418/4/2196/18439487/mnras0418-2196.pdf
Reference34 articles.
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4. Resolving cosmic structure formation with the Millennium-II Simulation
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1. Compact to extended Lyman-α emitters in MAGPI: Strong blue-peak emission at z ≳ 3;Astronomy & Astrophysics;2023-12
2. Modelling of Lyman-alpha emitting galaxies and ionized bubbles at the epoch of reionization;Monthly Notices of the Royal Astronomical Society;2018-04-21
3. Ly-α and Mg II as Probes of Galaxies and Their Environment;Publications of the Astronomical Society of the Pacific;2014-11
4. WHAT IS THE PHYSICAL ORIGIN OF STRONG Lyα EMISSION? I. DEMOGRAPHICS OF Lyα EMITTER STRUCTURES;The Astrophysical Journal;2014-03-26
5. FIRST SPECTROSCOPIC EVIDENCE FOR HIGH IONIZATION STATE AND LOW OXYGEN ABUNDANCE IN Lyα EMITTERS,;The Astrophysical Journal;2013-04-29
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