Takuya Hashimoto - Concepedia

Author

Takuya Hashimoto

National Astronomical Observatory of Japan ORCID

Also Known As

Hashimoto, T., Hashimoto, Takuya, T Hashimoto, T. Hashimoto, T. Sakamoto, T. Yoshii, Takuya Hashimoto, 橋本, 拓也

187

Publications

Citations

H-Index

Concepts

All Affiliations

National Astronomical Observatory of Japan The University of Tokyo University of Tsukuba Waseda University Centre National de la Recherche Scientifique

About

Takuya Hashimoto is an author at National Astronomical Observatory of Japan specializing in engineering, physics, and photometry.

Top Concepts

#	Concept	H-Index	Publications	Citations
1	Engineering	11	12	961
2	Natural Sciences	3	3	150
3	Health Sciences	1	1	16
4	Language Studies	1	1	16
5	Applied Physics	1	1	32

Takuya Hashimoto

Publications

3.8K

Citations

H-Index

Page 1

	Year	Citations
The onset of star formation 250 million years after the Big Bang Takuya Hashimoto, Nicolas Laporte, Ken Mawatari, Nature Galaxy FormationPhotometryEngineeringPhysicsCosmology	2018	340
Big Three Dragons: A <i>z</i> = 7.15 Lyman-break galaxy detected in [O <scp>iii</scp>] 88 μm, [C <scp>ii</scp>] 158 μm, and dust continuum with ALMA Takuya Hashimoto, Akio Inoue, Ken Mawatari, Publications of the Astronomical Society of Japan Cosmic AbundanceGalaxy FormationPhotometryEngineeringPhysics	2019	236
The MUSE <i>Hubble </i>Ultra Deep Field Survey Floriane Leclercq, Roland Bacon, L. Wisotzki, Astronomy and Astrophysics	2017	227
Detection of the Far-infrared [O iii] and Dust Emission in a Galaxy at Redshift 8.312: Early Metal Enrichment in the Heart of the Reionization Era Yoichi Tamura, Ken Mawatari, Takuya Hashimoto, The Astrophysical Journal	2019	211
Large Population of ALMA Galaxies at z > 6 with Very High [O iii] 88 μm to [C ii] 158 μm Flux Ratios: Evidence of Extremely High Ionization Parameter or PDR Deficit? Yuichi Harikane, Masami Ouchi, Akio Inoue, The Astrophysical Journal	2020	176
The MUSE <i>Hubble </i>Ultra Deep Field Survey Hanae Inami, Roland Bacon, J. Brinchmann, Astronomy and Astrophysics	2017	168
WHAT IS THE PHYSICAL ORIGIN OF STRONG Lyα EMISSION? II. GAS KINEMATICS AND DISTRIBUTION OF Lyα EMITTERS Takatoshi Shibuya, Masami Ouchi, Kimihiko Nakajima, The Astrophysical Journal	2014	152
ALMA uncovers the [C <scp>ii</scp>] emission and warm dust continuum in a <i>z</i> = 8.31 Lyman break galaxy Tom J. L. C. Bakx, Yoichi Tamura, Takuya Hashimoto, Monthly Notices of the Royal Astronomical Society	2020	148
FIRST SPECTROSCOPIC EVIDENCE FOR HIGH IONIZATION STATE AND LOW OXYGEN ABUNDANCE IN Lyα EMITTERS, Kimihiko Nakajima, Masami Ouchi, Kazuhiro Shimasaku, The Astrophysical Journal	2013	119
Recovering the systemic redshift of galaxies from their Lyman alpha line profile Anne Verhamme, Thibault Garel, E. Ventou, Monthly Notices of the Royal Astronomical Society Letters	2018	118

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