TH
Takuya Hashimoto
University of Tsukuba, Osaka Sangyo University, NAOJ, The University of Tokyo, 自然科学研究機構国立天文台/National Astronomical Observatory of Japan
Research areas: Physics and Astronomy · Astronomy and Astrophysics · Galaxies: Formation, Evolution, Phenomena · Astrophysics and Star Formation Studies · Stellar, planetary, and galactic studies
0000-0002-0898-4038
Employment
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University of Tsukuba Tenure-track assistant professor2019 - Present
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University of Tsukuba Assistant Professor2019 - Present
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自然科学研究機構国立天文台/National Astronomical Observatory of Japan 特任研究員/Project Researcher2019 - 2019
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Osaka Sangyo University, NAOJ2017 - Present
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University of Lyon, CRAL2015 - 2016
Education
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The University of Tokyo Ph.D.2012 - 2015
- 2010 - 2012
Projects & Funding
Projects & funding information is unavailable.
Publications (67)
- ALMA observations of pre-JWSTz ∼ 10 galaxy candidates: A CO(J = 9–8) line from a ULIRG at z = 2.54 and revisit of the photometric redshifts with JWST photometry Save
- ALMA Observations of [O i] 145 μm and [N ii] 205 μm Emission Lines from Star-forming Galaxies at z ∼ 7 Save
- ATT12: The Antarctic 12 m terahertz telescope for studies of dusty galaxies. I. Instrument sensitivity and science forecasts Save
- RIOJA. A Clumpy Galaxy Assembly at Redshift 6.81 Revealed by JWST Save
- RIOJA. Young starburst and ionized gas outflows in a z = 7.212 galaxy uncovered by JWST NIRCam and NIRSpec observations Save
- The first direct imaging of the silhouette of a damped Lyman α system along the line-of-sight to a background galaxy Save
- RIOJA. JWST and ALMA Unveil the Inhomogeneous and Complex Interstellar Medium Structure in a Star-forming Galaxy at z = 6.81 Save
- Compact Ionized Gas Region Surrounded by Porous Neutral Gas in a Dusty Lyman Break Galaxy at Redshift z = 8.312 Save
- RIOJA. Complex Dusty Starbursts in a Major Merger B14-65666 at z = 7.15 Save
- No Galaxy-scale [C ii] Fast Outflow in the z = 6.72 Red Quasar HSC J1205–0000 Save
- Detection of the [O i] 63 µm emission line from the z = 6.04 quasar J2054–0005 Save
- JWST/NIRSpec spectroscopy of intermediate-mass quiescent galaxies at z ~ 3-4 Save
- SERENADE. II. An ALMA Multiband Dust Continuum Analysis of 28 Galaxies at 5 < z < 8 and the Physical Origin of the Dust Temperature Evolution Save
- Gas conditions of a star-formation selected sample in the first billion years Save
- Molecular Outflow in the Reionization-epoch Quasar J2054-0005 Revealed by OH 119 μm Observations Save
- FOREVER22: the first bright galaxies with Population III stars at redshifts z ≃ 10–20 and comparisons with JWST data Save
- 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 Save
- Big Three Dragons: Molecular Gas in a Bright Lyman-break Galaxy at z = 7.15 Save
- 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 Save
- 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* Save