The physical origin for spatially large scatter of IGM opacity at the end of reionization: The IGM Lyα opacity-galaxy density relation
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N. Kashikawa | M. Onoue | T. Misawa | D. Kashino | T. Yoshioka | H. Uchiyama | Zheng Cai | Kei Ito | Rikako Ishimoto | K. Okoshi | Yongming Liang | Yoshihiro Takeda