The Physical Origin of Extreme Emission Line Galaxies at High Redshifts: Strong [O <scp>iii</scp>] Emission Lines Produced by Obscured Active Galactic Nuclei
Chenghao Zhu, Malte Schramm(Saitama University), Miftahul Hilmi(The University of Tokyo), Tohru Nagao(Ehime University), Masami Ouchi(Kavli Institute for the Physics and Mathematics of the Universe), Jenny E. Greene(The University of Tokyo), Yuichi Harikane(The University of Tokyo), Yoshiaki Ono(The University of Tokyo), Shenli Tang, Kazuhiro Shimasaku(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), Dongsheng Sun, Yechi Zhang(California Institute of Technology), Kimihiko Nakajima(National Astronomical Observatory of Japan), Masato Onodera(ETH Zurich), K. Iwasawa(Institució Catalana de Recerca i Estudis Avançats), Toshihiro Kawaguchi(Onomichi City University)
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