Yoshiki Matsuoka

Ehime University

Japan

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Articles (11)

Year:

2025

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2025

Year:

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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2024

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2024

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2023

Collaborators (15)

Jun Toshikawa

University of Bath

UNITED KINGDOM

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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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Hiroyuki Tashiro

Sojo University

JAPAN

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Marcin Sawicki

Professor

Saint Mary's University

CANADA

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Masayuki Akiyama

Associate Professor

Tohoku University

JAPAN

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Takuya Hashimoto

Assistant Professor

University of Tsukuba

JAPAN

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Kotaro Kohno

The Univeristy of Tokyo

JAPAN

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Nobunari Kashikawa

The Univeristy of Tokyo

JAPAN

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John Silverman

Professor

Kavli Institute for the Physics and Mathematics of the Universe

JAPAN

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Hideki Umehata

Nagoya University

JAPAN

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Tohru Nagao

Ehime University

JAPAN

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Satoshi Kikuta

University of Tokyo

JAPAN

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Masafusa Onoue

Assistant Professor

Waseda University

JAPAN

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Michael Strauss

Professor, Associate Chair

Princeton University

UNITED STATES

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Masatoshi Imanishi

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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Yoshiki Matsuoka

Research Interests

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Articles (11)

SHELLQs. Bridging the Gap: JWST Unveils Obscured Quasars in the Most Luminous Galaxies at z > 6

A post-starburst pathway for the formation of massive galaxies and black holes at z > 6

No Galaxy-scale [C ii] Fast Outflow in the z = 6.72 Red Quasar HSC J1205–0000

Subaru High-z Exploration of Low-luminosity Quasars (SHELLQs). XXI. Candidate Red Quasars at z ≥ 6 from Near-infrared Photometry

Subaru High-z Exploration of Low-Luminosity Quasars (SHELLQs) – XXIII. The powering mechanisms of the Lyα haloes around high-z quasars probed by slit spectroscopy

The Physical Origin of Extreme Emission Line Galaxies at High Redshifts: Strong [O iii] Emission Lines Produced by Obscured Active Galactic Nuclei

Merging Gas-rich Galaxies That Harbor Low-luminosity Twin Quasars at z = 6.05: A Promising Progenitor of the Most Luminous Quasars

Reconstruction of Cosmic Black Hole Growth and Mass Distribution from Quasar Luminosity Functions at z > 4: Implications for Faint and Low-mass Populations in JWST

The Relationship of Supermassive Black Holes and Host Galaxies at z < 4 in the Deep Optical Variability-selected Active Galactic Nuclei Sample in the COSMOS Field

Environments around Quasars at z ∼ 3 Revealed by Wide-field Imaging with Subaru HSC and CFHT

Evolution of the mass relation between supermassive black holes and dark matter halos across the cosmic time

Collaborators (15)

Jun Toshikawa

Takuma Izumi

Hiroyuki Tashiro

Marcin Sawicki

Masayuki Akiyama

Takuya Hashimoto

Kotaro Kohno

Nobunari Kashikawa

John Silverman

Hideki Umehata

Tohru Nagao

Satoshi Kikuta

Masafusa Onoue

Michael Strauss

Masatoshi Imanishi

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