HASHIMOTO Takuya
- Articles
- 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 - What is the Physical Origin of Strong Lyα Emission? I. Demographics of Lyα Emitter Structures
Shibuya Takatoshi; Ouchi Masami; Nakajima Kimihiko; Yuma ...
The Astrophysical Journal/785(1)/p.64, 2014-04 - First Spectroscopic Evidence for High Ionization State and Low Oxygen Abundance in Lyα Emitters
Nakajima Kimihiko; Ouchi Masami; Shimasaku Kazuhiro; Hash...
The Astrophysical Journal/769(1)/p.3, 2013-05 - Gas Motion Study of Lyα Emitters at z ~ 2 Using FUV and Optical Spectral Lines
Hashimoto Takuya; Ouchi Masami; Shimasaku Kazuhiro; Ono ...
The Astrophysical Journal/765(1)/p.70, 2013-03
- A Close Comparison between Observed and Modeled Lyα Lines for z ~ 2.2 Lyα Emitters