J-GLOBAL ID:201901016856214078   Update date: Sep. 01, 2020

Ishigaki Miho N

Ishigaki Miho N
Affiliation and department:
Research field  (1): Astronomy
Research keywords  (5): dark matter ,  chemical evolution ,  galaxy formation ,  nucleosynthesis ,  stellar spectroscopy
Research theme for competitive and other funds  (2):
  • 2017 - 2019 金属欠乏星の大規模化学組成解析に基づく銀河系恒星ハロー形成過程の解明
  • 2011 - 2012 球状星団の化学元素組成に基づく宇宙初期の銀河系形成過程の解明
MISC (25):
  • 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
  • Rana Ezzeddine, Anna Frebel, Ian U. Roederer, Nozomu Tominaga, Jason Tumlinson, Miho Ishigaki, Ken'ichi Nomoto, Vinicius M. Placco, Wako Aoki. Evidence for an aspherical Population III supernova explosion inferred from the hyper metal-poor star HE1327-2326. 2019
  • Tilman Hartwig, Miho N. Ishigaki, Ralf S. Klessen, Naoki Yoshida. Fingerprint of the first stars: multi-enriched extremely metal-poor stars in the TOPoS survey. 2018
  • Xilong Liang, Jingkun Zhao, Gang Zhao, Wako Aoki, Ishigaki Miho, Matsuno Tadafumi, Yuqin Chen, Xiaoming Kong, Jianrong Shi, Qianfan Xing. Tracing the origin of moving groups I. The γ Leo moving group with high resolution spectra from the Subaru Telescope. ApJ 2018. 863. 2018
  • Tilman Hartwig, Naoki Yoshida, Mattis Magg, Anna Frebel, Simon C.O. Glover, Facundo A. Gómez, Brendan Griffen, Miho N. Ishigaki, Alexander P. Ji, Ralf S. Klessen, et al. Descendants of the first stars: The distinct chemical signature of second-generation stars. Monthly Notices of the Royal Astronomical Society. 2018. 478. 2. 1795-1810
Lectures and oral presentations  (20):
  • 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)
Education (3):
  • 2007 - 2010 Tohoku University Astronomical Institute
  • 2005 - 2007 Tokyo Institute of Technology Physics
  • 2001 - 2005 International Christian University Natural Science Division
Work history (4):
  • 2019/02 - 現在 Tohoku University Astronomical Institute Postodoctoral Fellow
  • 2015/09 - 2019/01 University of Tokyo Kavli Institute for the Physics and Mathematics of the Universe Project Researcher
  • 2013/04 - 2015/08 University of Tokyo Kavli Institute for the Physics and Mathematics of the Universe JSPS fellow
  • 2010/04 - 2013/03 National Astronomical Observatory of Japan Hawaii Observatory Project Researcher
Awards (1):
  • 2016 - 東北大学理学部物理系同窓会「泉萩会」奨励賞 泉萩会奨励賞 銀河系の古成分恒星系の化学動力学に基づく銀河系の形成と進化の研究
Association Membership(s) (1):
※ Researcher’s information displayed in J-GLOBAL is based on the information registered in researchmap. For details, see here.

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