The Physical Origin of Extreme Emission Line Galaxies at High redshifts: Strong {\sc [Oiii]} Emission Lines Produced by Obscured AGNs
Chenghao Zhu, Malte Schramm(Saitama University), Jenny Greene, Toshihiro Kawaguchi(Onomichi City University), Miftahul Hilmi(The University of Tokyo), Tohru Nagao(Ehime University), Masami Ouchi(Kavli Institute for the Physics and Mathematics of the Universe), Yuichi Harikane(The University of Tokyo), Yoshiaki Ono(The University of Tokyo), Hiroya Umeda(Bunkyo University), Yoshiki Matsuoka(Ehime University), Yongming Liang(The Graduate University for Advanced Studies, SOKENDAI), Andreas Schulze, Kotaro Kohno(The University of Tokyo), Yuki Isobe(University of Cambridge), Yi Xu(Kavli Institute for the Physics and Mathematics of the Universe), Takatoshi Shibuya(Kitami Institute of Technology), Dong‐Sheng Sun, Yechi Zhang(California Institute of Technology), Kimihiko Nakajima(National Astronomical Observatory of Japan), Kazushi Iwasawa, Masato Onodera(ETH Zurich), Kazuhiro Shimasaku(Tokyo University of Science), Shenli Tang
Cited by 0
Related Papers
(untitled)
|Portsmouth Research Portal (University of Portsmouth)|2005|2.6k
The First Release COSMOS Optical and Near‐IR Data and Catalog
|The Astrophysical Journal Supplement Series|2007|808
The Hyper Suprime-Cam SSP Survey: Overview and survey design
|Dipòsit Digital de la Universitat de Barcelona (Universitat de Barcelona)|2018|777
Second data release of the Hyper Suprime-Cam Subaru Strategic Program
|Publications of the Astronomical Society of Japan|2019|516
MORPHOLOGIES OF ∼190,000 GALAXIES AT <i>z</i> = 0–10 REVEALED WITH <i>HST</i> LEGACY DATA. I. SIZE EVOLUTION
|The Astrophysical Journal Supplement Series|2015|433