Identifying Lyman α emitters powered by AGNs
Author:
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnrasl/article-pdf/432/1/L6/3930282/slt023.pdf
Reference24 articles.
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3. Galaxy Size Evolution at High Redshift and Surface Brightness Selection Effects: Constraints from the Hubble Ultra Deep Field
4. High-[CLC][ITAL]z[/ITAL][/CLC] L[CLC]y[/CLC]α Emitters. I. A Blank-Field Search for Objects near Redshift [CLC][ITAL]z[/ITAL][/CLC] = 3.4 in and around the Hubble Deep Field and the Hawaii Deep Field SSA 22
5. Spectroscopic Properties of thez≈ 4.5 Lyα Emitters
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1. Distinguishing AGN from starbursts as the origin of double-peaked Lyman-alpha emitters in the reionization era;Astronomy & Astrophysics;2021-02
2. Modelling a bright z = 6 galaxy at the faint end of the AGN luminosity function;Monthly Notices of the Royal Astronomical Society;2020-04-20
3. Inferring the astrophysics of reionization and cosmic dawn from galaxy luminosity functions and the 21-cm signal;Monthly Notices of the Royal Astronomical Society;2019-01-09
4. Finding bright z ≥ 6.6 Ly α emitters with lensing: prospects for Euclid;Monthly Notices of the Royal Astronomical Society;2017-06-23
5. AB INITIO COSMOLOGICAL SIMULATIONS OF CR7 AS AN ACTIVE BLACK HOLE;The Astrophysical Journal;2016-09-14
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