The Initial Mass Function of the First Stars Inferred from Extremely Metal-poor Stars von Ishigaki, Miho N., Tominaga, Nozomu, Kobayashi, Chiaki, Nomoto, Ken'ichi

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Dark matter annihilation and decay from non-spherical dark halos in galactic dwarf satellites von Hayashi, Kohei, Ichikawa, Koji, Matsumoto, Shigeki, Ibe, Masahiro, Ishigaki, Miho N., Sugai, Hajime

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Top-heavy stellar mass distribution in galactic nuclei inferred from the universally high abundance ratio of [Fe/Mg] von Toyouchi, Daisuke, Inayoshi, Kohei, Ishigaki, Miho N, Tominaga, Nozomu

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Enrichment in r-process Elements from Multiple Distinct Events in the Early Draco Dwarf Spheroidal Galaxy von Tsujimoto, Takuji, Matsuno, Tadafumi, Aoki, Wako, Ishigaki, Miho N., Shigeyama, Toshikazu

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Fingerprint of the first stars: multi-enriched extremely metal-poor stars in the TOPoS survey von Hartwig, Tilman, Ishigaki, Miho N, Klessen, Ralf S, Yoshida, Naoki

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Inferring the velocity of early massive stars from the abundances of extremely metal-poor stars von Choplin, Arthur, Tominaga, Nozomu, Ishigaki, Miho N.

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Machine Learning Detects Multiplicity of the First Stars in Stellar Archaeology Data von Hartwig, Tilman, Ishigaki, Miho N., Kobayashi, Chiaki, Tominaga, Nozomu, Nomoto, Ken’ichi

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Descendants of the first stars: the distinct chemical signature of second-generation stars von Hartwig, Tilman, Yoshida, Naoki, Magg, Mattis, Frebel, Anna, Glover, Simon C O, Gómez, Facundo A, Griffen, Brendan, Ishigaki, Miho N, Ji, Alexander P, Klessen, Ralf S, O’Shea, Brian W, Tominaga, Nozomu

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Star Formation Timescales of the Halo Populations from Asteroseismology and Chemical Abundances von Matsuno, Tadafumi, Aoki, Wako, Casagrande, Luca, Ishigaki, Miho, Shi, Jianrong, Takata, Masao, Xiang, Maosheng, Yong, David, Li, Haining, Suda, Takuma, Xing, Qianfan, Zhao, Jingkun

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A NEW MILKY WAY SATELLITE DISCOVERED IN THE SUBARU/HYPER SUPRIME-CAM SURVEY von Homma, Daisuke, Chiba, Masashi, Okamoto, Sakurako, Komiyama, Yutaka, Tanaka, Masayuki, Tanaka, Mikito, Ishigaki, Miho N., Akiyama, Masayuki, Arimoto, Nobuo, Garmilla, José A., Lupton, Robert H., Strauss, Michael A., Furusawa, Hisanori, Miyazaki, Satoshi, Murayama, Hitoshi, Nishizawa, Atsushi J., Takada, Masahiro, Usuda, Tomonori, Wang, Shiang-Yu

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EMPRESS. XIII. Chemical Enrichment of Young Galaxies Near and Far at z ∼ 0 and 4–10: Fe/O, Ar/O, S/O, and N/O Measurements with a Comparison of Chemical Evolution Models von Watanabe, Kuria, Ouchi, Masami, Nakajima, Kimihiko, Isobe, Yuki, Tominaga, Nozomu, Suzuki, Akihiro, Ishigaki, Miho N., Nomoto, Ken’ichi, Takahashi, Koh, Harikane, Yuichi, Hatano, Shun, Kusakabe, Haruka, Moriya, Takashi J., Nishigaki, Moka, Ono, Yoshiaki, Onodera, Masato, Sugahara, Yuma

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Boötes. IV. A new Milky Way satellite discovered in the Subaru Hyper Suprime-Cam Survey and implications for the missing satellite problem von Homma, Daisuke, Chiba, Masashi, Komiyama, Yutaka, Tanaka, Masayuki, Okamoto, Sakurako, Tanaka, Mikito, Ishigaki, Miho N, Hayashi, Kohei, Arimoto, Nobuo, Carlsten, Scott G, Lupton, Robert H, Strauss, Michael A, Miyazaki, Satoshi, Torrealba, Gabriel, Wang, Shiang-Yu, Murayama, Hitoshi

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Searches for new Milky Way satellites from the first two years of data of the Subaru/Hyper Suprime-Cam survey: Discovery of Cetus III von Homma, Daisuke, Chiba, Masashi, Okamoto, Sakurako, Komiyama, Yutaka, Tanaka, Masayuki, Tanaka, Mikito, Ishigaki, Miho N, Hayashi, Kohei, Arimoto, Nobuo, Garmilla, José A, Lupton, Robert H, Strauss, Michael A, Miyazaki, Satoshi, Wang, Shiang-Yu, Murayama, Hitoshi

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Origin of metals in old Milky Way halo stars based on GALAH and Gaia von Ishigaki, Miho N, Hartwig, Tilman, Tarumi, Yuta, Leung, Shing-Chi, Tominaga, Nozomu, Kobayashi, Chiaki, Magg, Mattis, Simionescu, Aurora, Nomoto, Ken’ichi

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Low [O/Fe] Ratio in a Luminous Galaxy at the Early Cosmic Epoch (z > 10): Signature of Short Delay Time or Bright Hypernovae/Pair-instability Supernovae? von Nakane, Minami, Ouchi, Masami, Nakajima, Kimihiko, Harikane, Yuichi, Tominaga, Nozomu, Takahashi, Koh, Kashino, Daichi, Yanagisawa, Hiroto, Watanabe, Kuria, Nomoto, Ken’ichi, Isobe, Yuki, Nishigaki, Moka, Ishigaki, Miho N., Ono, Yoshiaki, Takeda, Yui

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Chemo-dynamical Evolution of Simulated Satellites for a Milky Way–like Galaxy von Hirai, Yutaka, Kirby, Evan N., Chiba, Masashi, Hayashi, Kohei, Anguiano, Borja, Saitoh, Takayuki R., Ishigaki, Miho N., Beers, Timothy C.

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Detection of a Spatially Extended Stellar Population in M33: A Shallow Stellar Halo? von Ogami, Itsuki, Komiyama, Yutaka, Chiba, Masashi, Tanaka, Mikito, Guhathakurta, Puragra, Kirby, Evan N., Wyse, Rosemary F. G., Filion, Carrie, Kirihara, Takanobu, Ishigaki, Miho N., Hayashi, Kohei

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Four-hundred Very Metal-poor Stars Studied with LAMOST and Subaru. III. Dynamically Tagged Groups and Chemodynamical Properties von Zhang, Ruizhi, Matsuno, Tadafumi, Li, Haining, Aoki, Wako, Xue, Xiang-Xiang, Suda, Takuma, Zhao, Gang, Chen, Yuqin, Ishigaki, Miho N., Shi, Jianrong, Xing, Qianfan, Zhao, Jingkun

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Transition Probabilities of Near-infrared Ce iii Lines from Stellar Spectra: Applications to Kilonovae von Domoto, Nanae, Lee, Jae-Joon, Tanaka, Masaomi, Lee, Ho-Gyu, Aoki, Wako, Ishigaki, Miho N., Wanajo, Shinya, Kato, Daiji, Hotokezaka, Kenta

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Existence of tidal tails for the globular cluster NGC 5824 von Yang, Yong, Zhao, Jing-Kun, Ishigaki, Miho N., Chiba, Masashi, Yang, Cheng-Qun, Xue, Xiang-Xiang, Ye, Xian-Hao, Zhao, Gang

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