Hiroshi Matsuo

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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About

Hiroshi Matsuo is an Associate Professor at the National Astronomical Observatory of Japan. His research focuses on early universe galaxies, star formation processes, and terahertz photon detection technology. Recent publications explore topics such as ionized gas regions in distant galaxies and the conditions for star formation in the early cosmos. He is actively contributing to the understanding of the complex interactions of gas and dust in the universe.

Articles (16)

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2025

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2025

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2024

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2023

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2022

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2021

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2021

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2020

Collaborators (17)

Yuma Sugahara

講師(任期付)/Assistant Professor

Waseda University

JAPAN

Hiroshi Matsuo

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Articles (16)

Compact Ionized Gas Region Surrounded by Porous Neutral Gas in a Dusty Lyman Break Galaxy at Redshift z = 8.312

Detection of the [O i] 63 µm emission line from the z = 6.04 quasar J2054–0005

JWST, ALMA, and Keck Spectroscopic Constraints on the UV Luminosity Functions at z ∼ 7–14: Clumpiness and Compactness of the Brightest Galaxies in the Early Universe

RIOJA. Complex Dusty Starbursts in a Major Merger B14-65666 at z = 7.15

Recent Developments for the Terahertz Photon Detector System: Detector and Cryogenics

Development of 1.5 THz Photon Detectors for Terahertz Intensity Interferometry

Gas conditions of a star-formation selected sample in the first billion years

Erratum: “Possible Systematic Rotation in the Mature Stellar Population of a z = 9.1 Galaxy” (2022, ApJL, 933, L19)

Updated Measurements of [O iii] 88 μm, [C ii] 158 μm, and Dust Continuum Emission from a z = 7.2 Galaxy

Big Three Dragons: Molecular Gas in a Bright Lyman-break Galaxy at z = 7.15

Detections of [C ii] 158 μm and [O iii] 88 μm in a Local Lyman Continuum Emitter, Mrk 54, and Its Implications to High-redshift ALMA Studies*

Possible Systematic Rotation in the Mature Stellar Population of a z = 9.1 Galaxy

ALMA Reveals Extended Cool Gas and Hot Ionized Outflows in a Typical Star-forming Galaxy at Z = 7.13

Big Three Dragons: A [N ii] 122 μm Constraint and New Dust-continuum Detection of a z = 7.15 Bright Lyman-break Galaxy with ALMA

A puzzling non-detection of [O III] and [C II] from a z ≈ 7.7 galaxy observed with ALMA

Optical Performance of SIS Photon Detectors at Terahertz Frequencies

Collaborators (17)

Yuma Sugahara

Nicolas Laporte

Naoki Yoshida

Richard Ellis

Y Fudamoto

Kristian M Finlator

NARIO KUNO

Takuya Hashimoto

Tomonari Michiyama

Kana Moriwaki

Akio Inoue

Hideki Umehata

Tom Bakx

Santiago Arribas

Yoichi Tamura

Shigetomo Shiki

Seiji Fujimoto

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A puzzling non-detection of [O III] and [C II] from a z ≈ 7.7 galaxy observed with ALMA