The Physical Origin of Extreme Emission Line Galaxies at High Redshifts: Strong [O iii] Emission Lines Produced by Obscured Active Galactic Nuclei
Chenghao Zhu, Malte Schramm(Saitama University), Hiroya Umeda(Bunkyo University), Andreas Schulze, Takatoshi Shibuya(Kitami Institute of Technology), Yoshiaki Ono, Toshihiro Kawaguchi, Masato Onodera, Yechi Zhang, Yongming Liang, Jenny Greene, Kotaro Kohno, Masami Ouchi, Dongsheng Sun, Yi Meng Xu, Kazushi Iwasawa, Yuichi Harikane, Tohru Nagao, Yoshiki Matsuoka, Shenli Tang, Kimihiko Nakajima, Miftahul Hilmi(The University of Tokyo), Yuki Isobe, Kazuhiro Shimasaku(The University of Tokyo)
Institutional Repositories DataBase (IRDB)
March 12, 2025
Cited by 0
Related Papers
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
Third data release of the Hyper Suprime-Cam Subaru Strategic Program
|Publications of the Astronomical Society of Japan|2021|357
Big Three Dragons: A <i>z</i> = 7.15 Lyman-break galaxy detected in [O <scp>iii</scp>] 88 μm, [C <scp>ii</scp>] 158 μm, and dust continuum with ALMA
|Publications of the Astronomical Society of Japan|2019|245
COMPLETING THE CENSUS OF Lyα EMITTERS AT THE REIONIZATION EPOCH $^,$
|The Astrophysical Journal|2011|242