Miho N. Ishigaki (0000-0003-4656-0241)

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Miho N. Ishigaki is an Assistant Professor at the Subaru Telescope (Mitaka campus) in the National Astronomical Observatory of Japan. Her research topics are centered around the formation and evolution of our Milky Way Galaxy. She specifically interested in the origin of chemical elements in the Universe through high-resolution spectroscopy of very old stars in our Galaxy.

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自然科学研究機構国立天文台/National Astronomical Observatory of Japan: 三鷹市/Mitaka City, 東京都/Tokyo, JP

2020-05-01 to present | 助教/Assistant Professor (ハワイ観測所/Subaru Telescope)

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Miho N. Ishigaki

https://orcid.org/0000-0003-4656-0241

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Employment (6)

自然科学研究機構国立天文台/National Astronomical Observatory of Japan: 三鷹市/Mitaka City, 東京都/Tokyo, JP

Tohoku University: Sendai, Miyagi, JP

Tohoku University: Sendai, Miyagi, JP

Kavli Institute for the Physics and Mathematics of the Universe: Kashiwa, Chiba, JP

Kavli Institute for the Physics and Mathematics of the Universe: Kashiwa, Chiba, JP

National Astronomical Observatory of Japan: Mitaka, Tokyo, JP

Education and qualifications (3)

Tohoku University: Sendai, Miyagi, JP

Tokyo Institute of Technology: Meguro, Tokyo, JP

International Christian University: Mitaka, Tokyo, JP

Professional activities (1)

Astronomical Society of Japan: Mitaka, Tokyo, JP

Funding (2)

The formation of the Milky Way halo probed by statistical samples of elemental abundances in metal-poor stars

Revealing the early phase of the Milky Way Formation based on chemical abundances in globular clusters

Works (50 of 80)

A pristine view of galactic globular clusters and their peripheries: Omega Centauri

Chemo-dynamical Evolution of Simulated Satellites for a Milky Way–like Galaxy

Detection of a Spatially Extended Stellar Population in M33: A Shallow Stellar Halo?

Four-hundred Very Metal-poor Stars Studied with LAMOST and Subaru. III. Dynamically Tagged Groups and Chemodynamical Properties

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

Transition Probabilities of Near-infrared Ce iii Lines from Stellar Spectra: Applications to Kilonovae

Cerium Features in Kilonova Near-infrared Spectra: Implication from a Chemically Peculiar Star

Machine Learning Detects Multiplicity of the First Stars in Stellar Archaeology Data

Metal production in the early Universe: what chemical abundances in old stellar populations in the Milky Way tell us

Existence of tidal tails for the globular cluster NGC 5824

Four-hundred Very Metal-poor Stars Studied with LAMOST and Subaru. I. Survey Design, Follow-up Program, and Binary Frequency

Four-hundred Very Metal-poor Stars Studied with LAMOST and Subaru. II. Elemental Abundances

Revisit NGC 5466 tidal stream with Gaia, SDSS/SEGUE, and LAMOST

Top-heavy stellar mass distribution in galactic nuclei inferred from the universally high abundance ratio of [Fe/Mg]

Origin of metals in old Milky Way halo stars based on GALAH and Gaia

Star Formation Timescales of the Halo Populations from Asteroseismology and Chemical Abundances*

Evidence for the Third Stellar Population in the Milky Way’s Disk

Bo\"otes IV: A New Milky Way Satellite Discovered in the Subaru Hyper Suprime-Cam Survey and Implications for the Missing Satellite Problem

Chemical abundances of field halo stars - Implications for the building blocks of the Milky Way

Evidence for an Aspherical Population III Supernova Explosion Inferred from the Hyper-metal-poor Star HE 1327─2326

Evidence for the accretion origin of halo stars with an extreme r-process enhancement

Evidence for the third stellar population in the Milky Way's disk

Constraints on the chemical enrichment history of the Perseus Cluster of galaxies from high-resolution X-ray spectroscopy

VizieR Online Data Catalog: Modelled vs observed abundances of EMP stars (Ishigaki+, 2018)

Fingerprint of the first stars: multi-enriched extremely metal-poor stars in the TOPoS survey

Line identification and photometric history of the hot post-AGB star Hen 3-1013 (IRAS 14331-6435)

Tracing the Origin of Moving Groups. II. Chemical Abundance of Six Stars in the Halo Stream LAMOST-N1

LAMOST J221750.59+210437.2: A new member of carbon-enhanced extremely metal-poor stars with excesses of Mg and Si

Foreground effect on the J-factor estimation of ultrafaint dwarf spheroidal galaxies

Descendants of the first stars: the distinct chemical signature of second-generation stars

Tracing the Origin of Moving Groups. I. The γ Leo Moving Group with High-resolution Spectra from the Subaru Telescope

Optical High-resolution Spectroscopy of 14 Young α-rich Stars

The Initial Mass Function of the First Stars Inferred from Extremely Metal-poor Stars

Searches for new Milky Way satellites from the first two years of data of the Subaru/Hyper Suprime-Cam survey: Discovery of Cetus III

Photometric Identification of Population III Core-Collapse Supernovae: Multicolor Light Curve Simulations

Core-Collapse Supernovae in the Early Universe: Radiation Hydrodynamics Simulations of Multicolor Light Curves

Enrichment in r-process Elements from Multiple Distinct Events in the Early Draco Dwarf Spheroidal Galaxy

Foreground effect on the J-factor estimation of classical dwarf spheroidal galaxies

A New Milky Way Satellite Discovered in the Subaru/Hyper Suprime-Cam Survey

Dark matter annihilation and decay from non-spherical dark halos in galactic dwarf satellites

Chemical evolution of r-process elements in the Draco dwarf spheroidal galaxy

VizieR Online Data Catalog: LOS velocities &amp; [Fe/H] of Pal 5 tidal stream (Ishigaki+, 2016)

Line-of-sight Velocity and Metallicity Measurements of the Palomar 5 Tidal Stream

Multicolor Light Curve Simulations of Population III Core-Collapse Supernovae: From Shock Breakout to <SUP>56</SUP>Co Decay

Sodium Absorption Systems toward SN Ia 2014J Originate on Interstellar Scales

Type IIb Supernova 2013df Entering into an Interaction Phase: A Link between the Progenitor and the Mass Loss

Chemical feature of Eu abundance in the Draco dwarf spheroidal galaxy<SUP>†</SUP>

Stellar Abundances for Galactic Archaeology database for stars in dwarf galaxies

Faint Population III Supernovae as the Origin of the Most Iron-poor Stars

The Origin of Low [α/Fe] Ratios in Extremely Metal-poor Stars

VizieR Online Data Catalog: LOS velocities & [Fe/H] of Pal 5 tidal stream (Ishigaki+, 2016)