Takuya Hashimoto

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Assistant Professor

University of Tsukuba

Japan

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Dr. Takuya Hashimoto is an Assistant Professor at the University of Tsukuba, Japan. His research interests focus on the interstellar medium and galaxy formation, as evidenced by his recent publications, including works on the complex structures of star-forming galaxies at high redshifts and the conditions in early galaxies. His contributions also include studies on ionized gas regions and the physical processes associated with galaxy evolution during the reionization epoch.

Recent Grants

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JSPS Research Fellowship for Young Scientists

Open Date: 2014-04-01

Close Date: 2016-03-01

Takuya Hashimoto

Research Interests

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Recent Grants

Articles (20)

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

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

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

RIOJA. JWST and ALMA Unveil the Inhomogeneous and Complex Interstellar Medium Structure in a Star-forming Galaxy at z = 6.81

The first direct imaging of the silhouette of a damped Lyman α system along the line-of-sight to a background galaxy

SERENADE. II. An ALMA Multiband Dust Continuum Analysis of 28 Galaxies at 5 < z < 8 and the Physical Origin of the Dust Temperature Evolution

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

Molecular Outflow in the Reionization-epoch Quasar J2054-0005 Revealed by OH 119 μm Observations

JWST/NIRSpec spectroscopy of intermediate-mass quiescent galaxies at z ~ 3-4

The 300 pc Resolution Imaging of a z = 8.31 Galaxy: Turbulent Ionized Gas and Potential Stellar Feedback 600 Million Years after the Big Bang

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*

FOREVER22: the first bright galaxies with Population III stars at redshifts z ≃ 10–20 and comparisons with JWST data

Reionization and the ISM/Stellar Origins with JWST and ALMA (RIOJA): The Core of the Highest-redshift Galaxy Overdensity at z = 7.88 Confirmed by NIRSpec/JWST

H1821+643: The Most X-Ray and Infrared Luminous Active Galactic Nucleus (AGN) in the Swift/BAT Survey in the Process of Rapid Stellar and Supermassive Black Hole Mass Assembly

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

Bridging Optical and Far-infrared Emission-line Diagrams of Galaxies from Local to the Epoch of Reionization: Characteristic High [O iii] 88 μm/SFR at z > 6

Collaborators (24)

Hajime Fukushima

Yuma Sugahara

Nicolas Laporte

Naoki Yoshida

Takuma Izumi

Takashi Okamoto

Y Fudamoto

Kristian M Finlator

NARIO KUNO

Yoshiki Matsuoka

Bunyo Hatsukade

Masayuki Akiyama

Tomonari Michiyama

Hiroshi Matsuo

RHYTHM SHIMAKAWA

Kana Moriwaki

Hideki Umehata

Tom Bakx

Yusuke MIYAMOTO

Santiago Arribas

Yoichi Tamura

Seiji Fujimoto

Michael Strauss

Masatoshi Imanishi

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