ASAGAO. Average Morphology of High-$z$ Dusty Star-Forming Galaxies is an Exponential-Disk ($n \simeq 1$) Harboring an AGN

Seiji Fujimoto(Waseda University), Yoichi Tamura(Nagoya University), Bunyo Hatsukade(The University of Tokyo), Wei-Hao Wang(Institute of Astronomy and Astrophysics, Academia Sinica), Shigeki Inoue(Kavli Institute for the Physics and Mathematics of the Universe), Ichi Tanaka(Subaru (Japan)), Taira Oogi(Kavli Institute for the Physics and Mathematics of the Universe), Yiping Ao(Chinese Academy of Sciences), Tao Wang(National Astronomical Observatory of Japan), D. Espada(The Graduate University for Advanced Studies, SOKENDAI), Tohru Nagao(Ehime University), Yoshiaki Taniguchi(Higashiosaka College & Higashiosaka Junior College), Ken-ichi Tadaki(National Astronomical Observatory of Japan), Masami Ouchi(Kavli Institute for the Physics and Mathematics of the Universe), W. Rujopakarn(Chulalongkorn University), Yoshihiro Ueda(Kyoto University), Hideki Umehata(The Open University of Japan), Kouichiro Nakanishi(JCR Pharmaceuticals (Japan)), Sune Toft(University of Copenhagen), Kotaro Kohno(The University of Tokyo), Minju Lee(National Astronomical Observatory of Japan), Takatoshi Shibuya(Kitami Institute of Technology), Yuki Yamaguchi(The University of Tokyo), J. Ivison, Carlos Gómez-Guijarro(Centre National de la Recherche Scientifique)

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February 6, 2018

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