Hashimoto Takuya

Researcher's full information

Articles

• 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?
  Harikane Yuichi; Ouchi Masami; Inoue Akio K.; Matsuoka Y...
  The Astrophysical Journal/896(2)/pp.93-112, 2020-06
• ALMA uncovers the [C II] emission and warm dust continuum in a z = 8.31 Lyman break galaxy
  Bakx Tom J. L. C.; Tamura Yoichi; Hashimoto Takuya; Inoue...
  Monthly Notices of the Royal Astronomical Society/493(3)/pp.4294-4307, 2020-04
• Elevated ionizing photon production efficiency in faint high-equivalent-width Lyman-α emitters
  Maseda Michael V.; Bacon Roland; Lam Daniel; Matthee Jor...
  Monthly Notices of the Royal Astronomical Society/493(4)/pp.5120-5130, 2020-04
• The MUSE Hubble Ultra Deep Field Survey. XIII. Spatially resolved spectral properties of Lyman α haloes around star-forming galaxies at z > 3
  Leclercq Floriane; Bacon Roland; Verhamme Anne; Garel Th...
  Astronomy & Astrophysics/635, 2020-03
  
  Tsukuba Repository
• Balmer Break Galaxy Candidates at z ∼ 6: A Potential View on the Star Formation Activity at z ≳ 14
  Mawatari Ken; Inoue Akio K.; Hashimoto Takuya; Silverman ...
  The Astrophysical Journal/889(2), 2020-02
• Detections of [O III] 88 μm in two quasars in the reionization epoch
  Hashimoto Takuya; Inoue Akio K.; Tamura Yoichi; Matsuo H...
  Publications of the Astronomical Society of Japan/71(6)/p.109, 2019-12
• Balmer breaks in simulated galaxies at z > 6
  Binggeli Christian; Zackrisson Erik; Ma Xiangcheng; Inoue...
  Monthly Notices of the Royal Astronomical Society/489(3)/pp.3827-3835, 2019-11
• SILVERRUSH. VIII. Spectroscopic Identifications of Early Large-scale Structures with Protoclusters over 200 Mpc at z ̃ 6-7: Strong Associations of Dusty Star-forming Galaxies
  Harikane Yuichi; Ouchi Masami; Ono Yoshiaki; Fujimoto Se...
  The Astrophysical Journal/883(2)/p.142, 2019-10
• Big Three Dragons: A z = 7.15 Lyman-break galaxy detected in [O III] 88 μm, [C II] 158 μm, and dust continuum with ALMA
  Hashimoto Takuya; Inoue Akio K.; Mawatari Ken; Tamura Yo...
  Publications of the Astronomical Society of Japan/71(4)/p.71, 2019-08
• The absence of [C II] 158 μm emission in spectroscopically confirmed galaxies at z > 8
  Laporte N.; Katz H.; Ellis R. S.; Lagache G.; Bauer F. E...
  Monthly Notices of the Royal Astronomical Society: Letters/487(1)/pp.81-85, 2019-07
• The dominant origin of diffuse Lyα halos around Lyα emitters explored by spectral energy distribution fitting and clustering analysis
  Kusakabe Haruka; Shimasaku Kazuhiro; Momose Rieko; Ouchi ...
  Publications of the Astronomical Society of Japan/71(3)/p.55, 2019-06
• 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
  Tamura Yoichi; Mawatari Ken; Hashimoto Takuya; Inoue Aki...
  The Astrophysical Journal/874(1)/p.27, 2019-03
• The distribution and physical properties of high-redshift [O III] emitters in a cosmological hydrodynamics simulation
  Moriwaki Kana; Yoshida Naoki; Shimizu Ikkoh; Harikane Yu...
  Monthly Notices of the Royal Astronomical Society: Letters/481(1)/pp.84-88, 2018-11
• MUSE Spectroscopic Identifications of Ultra-faint Emission Line Galaxies with M UV ̃ -15
  Maseda Michael V.; Bacon Roland; Franx Marijn; Brinchmann...
  The Astrophysical Journal Letters/865(1), 2018-09
• Recovering the systemic redshift of galaxies from their Lyman alpha line profile
  Verhamme A.; Garel T.; Ventou E.; Contini T.; Bouché N.; ...
  Monthly Notices of the Royal Astronomical Society: Letters/478(1)/pp.60-65, 2018-07
• The onset of star formation 250 million years after the Big Bang
  Hashimoto Takuya; Laporte Nicolas; Mawatari Ken; Ellis R...
  Nature/557(7705)/pp.392-395, 2018-05
• The stellar mass, star formation rate and dark matter halo properties of LAEs at z ∼ 2
  Kusakabe Haruka; Shimasaku Kazuhiro; Ouchi Masami; Nakaji...
  Publications of the Astronomical Society of Japan/70(1)/p.4, 2018-01
• The MUSE Hubble Ultra Deep Field Survey. X. Lyα equivalent widths at 2.9 < z < 6.6
  Hashimoto Takuya; Garel T.; Guiderdoni B.; Drake A. B.; B...
  Astronomy & Astrophysics/608(10), 2017-11
• The MUSE Hubble Ultra Deep Field Survey. VI. The faint-end of the Lyα luminosity function at 2.91 < z < 6.64 and implications for reionisation
  Drake A. B.; Garel T.; Wisotzki L.; Leclercq F.; Hashimot...
  Astronomy & Astrophysics/608(A6), 2017-11
• The MUSE Hubble Ultra Deep Field Survey. II. Spectroscopic redshifts and comparisons to color selections of high-redshift galaxies
  Inami H.; Bacon R.; Brinchmann J.; Richard J.; Contini T...
  Astronomy & Astrophysics/608(A2), 2017-11
• The MUSE Hubble Ultra Deep Field Survey. VIII. Extended Lyman-α haloes around high-z star-forming galaxies
  Leclercq Floriane; Bacon Roland; Wisotzki Lutz; Mitchell ...
  Astronomy & Astrophysics/608(A8), 2017-11
• MUSE deep-fields: the Ly α luminosity function in the Hubble Deep Field-South at 2.91 < z < 6.64
  Drake Alyssa B.; Guiderdoni Bruno; Blaizot Jérémy; Wisotz...
  Monthly Notices of the Royal Astronomical Society/471(1)/pp.267-278, 2017-10
• Lyα emitters with very large Lyα equivalent widths, EW0(Lyα) ≃ 200-400 Å, at z ∼ 2
  Hashimoto Takuya; Ouchi Masami; Shimasaku Kazuhiro; Schae...
  Monthly Notices of the Royal Astronomical Society/465(2)/pp.1543-1562, 2017-02
• A Close Comparison between Observed and Modeled Lyα Lines for z ~ 2.2 Lyα Emitters
  Hashimoto Takuya; Verhamme Anne; Ouchi Masami; Shimasaku ...
  The Astrophysical Journal/812(2)/p.157, 2015-10
• What is the Physical Origin of Strong Lyα Emission? II. Gas Kinematics and Distribution of Lyα Emitters
  Shibuya Takatoshi; Ouchi Masami; Nakajima Kimihiko; Hashi...
  The Astrophysical Journal/788(1)/p.74, 2014-06
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