Three-dimensional Distribution Map of H i Gas and Galaxies around an Enormous Lyα Nebula and Three QSOs at z = 2.3 Revealed by the H i Tomographic Mapping Technique

Shiro Mukae(The University of Tokyo), Ryota Kakuma(The University of Tokyo), Khee‐Gan Lee(Kavli Institute for the Physics and Mathematics of the Universe), Joseph F. Hennawi(University of California, Santa Barbara), Toru Misawa(Pennsylvania State University), J. D. Silverman(Kavli Institute for the Physics and Mathematics of the Universe), J. X. Prochaska(Kavli Institute for the Physics and Mathematics of the Universe), Yuma Sugahara(Waseda University), Masami Ouchi(Kavli Institute for the Physics and Mathematics of the Universe), Yuichi Harikane(The University of Tokyo), Ken Mawatari(Osaka Sangyo University), N. Suzuki(Lawrence Berkeley National Laboratory), Kentaro Nagamine(University of Nevada, Las Vegas), Takashi Kojima(National Astronomical Observatory of Japan), Sebastiano Cantalupo(ETH Zurich), Zheng Cai, Akio Inoue(Osaka Sangyo University), Haibin Zhang(The University of Tokyo), Zheng Zheng(University of Utah), Takatoshi Shibuya(Kitami Institute of Technology), Yuichi Matsuda(The Graduate University for Advanced Studies, SOKENDAI), Yi-Kuan Chiang(Johns Hopkins University), Yoshiaki Ono(Kavli Institute for the Physics and Mathematics of the Universe), Seiji Fujimoto(Waseda University)
The Astrophysical Journal
June 1, 2020
Cited by 15


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