Masao Hayashi

特任助教/Project Assistant Professor

自然科学研究機構国立天文台/National Astronomical Observatory of Japan

Japan

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About

Masao Hayashi is a Project Assistant Professor at the National Astronomical Observatory of Japan. His research focuses on the study of gas properties in galaxies, star formation, and the environmental factors affecting these processes, as demonstrated in his recent publications utilizing ALMA and other observational data. He has contributed to understanding high-redshift galaxy formations and the impact of galactic morphology on gas content. His work also includes exploring the properties of extreme emission-line galaxies and the dynamics of star-forming regions in dense clusters.

Articles (10)

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2022

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2022

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2021

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2021

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2021

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2021

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2021

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2021

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2020

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2020

Collaborators (8)

Takuma Izumi

助教/Assistant Professor

自然科学研究機構国立天文台/National Astronomical Observatory of Japan

JAPAN

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Kazuhito Motogi

Lecturer

Yamaguchi University

JAPAN

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Bunyo Hatsukade

准教授/Associate Professor

自然科学研究機構国立天文台/National Astronomical Observatory of Japan

JAPAN

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Kotaro Niinuma

Prof.

Yamaguchi University

JAPAN

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RHYTHM SHIMAKAWA

Associate Professor

Waseda University

JAPAN

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Martha Haynes

Distinguished Professor of Arts and Sciences in Astronomy

Cornell University

UNITED STATES

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Masato Onodera

Assistant Professor

Graduate University for Advanced Studies

JAPAN

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Ken-ichi Tadaki

Hokkai Gakuen University

JAPAN

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Masao Hayashi

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Articles (10)

High-resolution ALMA Study of CO J = 2–1 Line and Dust Continuum Emissions in Cluster Galaxies at z = 1.46

The Environmental Dependence of Gas Properties in Dense Cores of a Protocluster at z ∼ 2.5 Revealed with ALMA

What Determines the H i Gas Content in Galaxies? Morphological Dependence of the H i Gas Fraction across the M *–SFR Plane

Dust, Gas, and Metal Content in Star-forming Galaxies at z ∼ 3.3 Revealed with ALMA and Near-IR Spectroscopy

Erratum: Extended star-forming region within galaxies in a dense proto-cluster core at z = 2.53

EMPRESS. II. Highly Fe-enriched Metal-poor Galaxies with ∼1.0 (Fe/O)⊙ and 0.02 (O/H)⊙: Possible Traces of Supermassive (>300 M ⊙) Stars in Early Galaxies* † ‡

Subaru Hyper Suprime-Cam excavates colossal over- and underdense structures over 360 deg2 out to z = 1

Variability of Late-time Radio Emission in the Superluminous Supernova PTF10hgi

Broadband Selection, Spectroscopic Identification, and Physical Properties of a Population of Extreme Emission-line Galaxies at 3 < z < 3.7

A 16 deg2 survey of emission-line galaxies at z < 1.6 from HSC-SSP PDR2 and CHORUS

Collaborators (8)

Takuma Izumi

Kazuhito Motogi

Bunyo Hatsukade

Kotaro Niinuma

RHYTHM SHIMAKAWA

Martha Haynes

Masato Onodera

Ken-ichi Tadaki

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Masao Hayashi

Research Interests

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About

Articles (10)

High-resolution ALMA Study of CO J = 2–1 Line and Dust Continuum Emissions in Cluster Galaxies at z = 1.46

The Environmental Dependence of Gas Properties in Dense Cores of a Protocluster at z ∼ 2.5 Revealed with ALMA

What Determines the H i Gas Content in Galaxies? Morphological Dependence of the H i Gas Fraction across the M *–SFR Plane

Dust, Gas, and Metal Content in Star-forming Galaxies at z ∼ 3.3 Revealed with ALMA and Near-IR Spectroscopy

Erratum: Extended star-forming region within galaxies in a dense proto-cluster core at z = 2.53

EMPRESS. II. Highly Fe-enriched Metal-poor Galaxies with ∼1.0 (Fe/O)⊙ and 0.02 (O/H)⊙: Possible Traces of Supermassive (>300 M ⊙) Stars in Early Galaxies* † ‡

Subaru Hyper Suprime-Cam excavates colossal over- and underdense structures over 360 deg2 out to z = 1

Variability of Late-time Radio Emission in the Superluminous Supernova PTF10hgi

Broadband Selection, Spectroscopic Identification, and Physical Properties of a Population of Extreme Emission-line Galaxies at 3 < z < 3.7

A 16 deg2 survey of emission-line galaxies at z &lt; 1.6 from HSC-SSP PDR2 and CHORUS

Collaborators (8)

Takuma Izumi

Kazuhito Motogi

Bunyo Hatsukade

Kotaro Niinuma

RHYTHM SHIMAKAWA

Martha Haynes

Masato Onodera

Ken-ichi Tadaki

Make your next move.

A 16 deg2 survey of emission-line galaxies at z < 1.6 from HSC-SSP PDR2 and CHORUS