Broadband Selection, Spectroscopic Identification, and Physical Properties of a Population of Extreme Emission-line Galaxies at 3 < z < 3.7

We present the selection, spectroscopic identification, and physical properties of extreme emission-line galaxies (EELGs) at 3 

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Bibliographic Details
Published in:The Astrophysical journal 2020-12, Vol.904 (2), p.180
Main Authors: Onodera, Masato, Shimakawa, Rhythm, Suzuki, Tomoko L., Tanaka, Ichi, Harikane, Yuichi, Hayashi, Masao, Kodama, Tadayuki, Koyama, Yusei, Nakajima, Kimihiko, Shibuya, Takatoshi
Format: Article
Language:English
Subjects:
Astrophysics
Attenuation
Broadband
Continuum modeling
Cosmic dust
Emission analysis
Emission lines
Emitters
Galaxies
H alpha line
Hydrogen
Interstellar matter
Interstellar medium
Ionization
Leakage
Metallicity
Physical properties
Spectroscopy
Spectrum analysis
Star & galaxy formation
Star formation
Stars
Stars & galaxies
Stellar models
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Description
Summary:We present the selection, spectroscopic identification, and physical properties of extreme emission-line galaxies (EELGs) at 3 
ISSN:0004-637X
1538-4357
DOI:10.3847/1538-4357/abc174