Wako Aoki, Haining Li, Tadafumi Matsuno, Qianfan Xing, Yuqin Chen, Norbert Christlieb, Satoshi Honda, Miho N. Ishigaki, Jianrong Shi, Takuma Suda, et al. Four-hundred Very Metal-poor Stars Studied with LAMOST and Subaru. I. Survey Design, Follow-up Program, and Binary Frequency. The Astrophysical Journal. 2022. 931. 2. 146-146
Haining Li, Wako Aoki, Tadafumi Matsuno, Qianfan Xing, Takuma Suda, Nozomu Tominaga, Yuqin Chen, Satoshi Honda, Miho N. Ishigaki, Jianrong Shi, et al. Four-hundred Very Metal-poor Stars Studied with LAMOST and Subaru. II. Elemental Abundances. The Astrophysical Journal. 2022. 931. 2. 147-147
Miho N. Ishigaki, Tilman Hartwig, Yuta Tarumi, Shing-Chi Leung, Nozomu Tominaga, Chiaki Kobayashi, Mattis Magg, Aurora Simionescu, Ken'ichi Nomoto. Origin of metals in old Milky Way halo stars based on GALAH and Gaia. Monthly Notices of the Royal Astronomical Society. 2021. 506. 4. 5410-5429
Tadafumi Matsuno, Wako Aoki, Luca Casagrande, Miho N. Ishigaki, Jianrong Shi, Masao Takata, Maosheng Xiang, David Yong, Haining Li, Takuma Suda, et al. Star Formation Timescales of the Halo Populations from Asteroseismology and Chemical Abundances. Astrophysical Journal. 2021. 912. 1
Tian Qiu, Wenting Wang, Masahiro Takada, Naoki Yasuda, Zeljko Ivezic, Robert H. Lupton, Masashi Chiba, Miho Ishigaki, Yutaka Komiyama. Proper motion measurements for stars up to 100 kpc with Subaru HSC and SDSS Stripe 82. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY. 2021. 501. 4. 5149-5175
Qian-Fan Xing, Gang Zhao, Wako Aoki, Satoshi Honda, Hai-Ning Li, Miho N. Ishigaki, Tadafumi Matsuno. Evidence for the accretion origin of halo stars with an extreme r-process enhancement. 2019
Daniela Carollo, Masashi Chiba, Miho Ishigaki, Ken Freeman, Chiara Battistini, Tim Beers, Patricia Tissera, Francesca Primas, Y. S. Lee. Evidence for the third stellar population in the Milky Way's disk. 2019
Chemical abundance patterns in the Milky Way halo stars as constraints on the element production in the early Universe
(EAO Subaru Science Workshop 2019 2019)
The initial mass function of the first stars inferred from elemental abundances in extremely metal-poor stars
(Stellar Archaeology as a Time Machine to the First Stars 2018)
Implications of Extremely Metal-Poor stars on the Masses of the First Stars
(A Celebration of CEMP and Gala of GALAH 2017)
EMP abundances compared with supernova yields of the Pop III stars
(The Japan-France Workshop “Neutron Star Mergers and Galactic Chemical Evolution” 2017)
EMP abundances compared with supernova yields of the Pop III stars
(Stellar Evolution, Supernova and Nucleosynthesis across Cosmic Time 2017)