Mariko Kubo

assistant professor

Tohoku University

Japan

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Mariko Kubo is an assistant professor at Tohoku University in Japan. Her research focuses on the dynamics of gas and star formation in galaxies, particularly within protoclusters at high redshifts. Recent publications include studies on the faint end of the far-infrared luminosity function and the properties of massive quiescent galaxies. She utilizes advanced observational techniques with facilities such as ALMA and JWST to explore the characteristics of galaxies in evolving cosmic environments.

Articles (18)

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2025

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2025

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2025

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2025

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2024

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2024

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2023

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2023

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2023

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2023

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2022

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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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2020

Collaborators (13)

Ian Smail

Professor

University of Durham

UNITED KINGDOM

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Jun Toshikawa

University of Bath

UNITED KINGDOM

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Ikuru Iwata

Associate Professor

National Astronomical Observatory of Japan

JAPAN

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Kohei Ichikawa

Assistant Professor

Tohoku University

JAPAN

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Erik Monson

Lecturer

Middle Tennessee State University

UNITED STATES

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Sune Toft

Københavns Universitet

DENMARK

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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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Kei Ito

University of Tokyo

JAPAN

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Masato Onodera

Assistant Professor

Graduate University for Advanced Studies

JAPAN

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Francesco Valentino

Københavns Universitet

DENMARK

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Hideki Umehata

Nagoya University

JAPAN

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Douglas Scott

University of British Columbia Faculty of Science

CANADA

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C M Harrison

Newcastle University

UNITED KINGDOM

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Mariko Kubo

Research Interests

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Articles (18)

ADF22+: A declining faint end in the far-infrared luminosity function in the SSA22 protocluster at z = 3.09

ADF22-WEB: Detection of a Molecular Gas Reservoir in a Massive Quiescent Galaxy Located in a z ≈ 3 Protocluster Core

Galaxy properties from the outskirts to the core of a protocluster at z = 3.70

Deciphering Gas Dynamics and Star Formation in a z = 1.1 Main-sequence Spiral Galaxy with ALMA and JWST

A Protocluster of Massive Quiescent Galaxies at z = 4

A Massive Quiescent Galaxy in a Group Environment at z = 4.53

COSMOS2020: Discovery of a Protocluster of Massive Quiescent Galaxies at z = 2.77

Revisiting the Properties of X-Ray Active Galactic Nuclei in the SSA22 Protocluster: Normal Supermassive Black Hole and Host-galaxy Growth for AGNs in a z = 3.09 Overdensity

An enhanced abundance of bright galaxies in protocluster candidates at z ∼ 3–5

New technique to select recent fast-quenching galaxies at z ~ 2 using the optical colours

An AGN with an Ionized Gas Outflow in a Massive Quiescent Galaxy in a Protocluster at z = 3.09

A Wide and Deep Exploration of Radio Galaxies with Subaru HSC (WERGS). VII. Redshift Evolution of Radio Galaxy Environments at z = 0.3–1.4

A Wide and Deep Exploration of Radio Galaxies with Subaru HSC (WERGS). VI. Distant Filamentary Structures Pointed Out by High-z Radio Galaxies at z ∼ 4

A Massive Quiescent Galaxy Confirmed in a Protocluster at z = 3.09

ALMA Observations of Lyα Blob 1: Multiple Major Mergers and Widely Distributed Interstellar Media

On the Nature of AGN and Star Formation Enhancement in the z = 3.1 SSA22 Protocluster: The HST WFC3 IR View

Interrelation of the Environment of Lyα Emitters and Massive Galaxies at 2 < z < 4.5

Testing an indirect method for identifying galaxies with high levels of Lyman continuum leakage

Collaborators (13)

Ian Smail

Jun Toshikawa

Ikuru Iwata

Kohei Ichikawa

Erik Monson

Sune Toft

Bunyo Hatsukade

Kei Ito

Masato Onodera

Francesco Valentino

Hideki Umehata

Douglas Scott

C M Harrison

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