EMPRESS. II. Highly Fe-enriched Metal-poor Galaxies with ∼1.0 (Fe/O)<sub>⊙</sub> and 0.02 (O/H)<sub>⊙</sub>: Possible Traces of Supermassive (>300 M <sub>⊙</sub>) Stars in Early Galaxies* † ‡
Takashi Kojima(National Astronomical Observatory of Japan), Kiyoto Yabe(Kavli Institute for the Physics and Mathematics of the Universe), Seiji Fujimoto(Waseda University), Shiro Mukae(The University of Tokyo), Chien‐Hsiu Lee(National Astronomical Observatory of Japan), Yuma Sugahara(Waseda University), Masao Hayashi(University of Tsukuba), Tohru Nagao(Ehime University), Masami Ouchi(Kavli Institute for the Physics and Mathematics of the Universe), Yutaka Komiyama(The Graduate University for Advanced Studies, SOKENDAI), Yuichi Harikane(The University of Tokyo), Yoshiaki Ono(The University of Tokyo), Masayuki Umemura(University of Tsukuba), Takuya Hashimoto(Université Claude Bernard Lyon 1), Haruka Kusakabe(The Graduate University for Advanced Studies, SOKENDAI), Yuki Isobe(University of Cambridge), Ji Hoon Kim(Seoul National University), Takatoshi Shibuya(Kitami Institute of Technology), Masato Onodera(ETH Zurich), Kimihiko Nakajima(National Astronomical Observatory of Japan), Michael Rauch(Carnegie Observatories)
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