PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN 71(3) 2019年6月
We investigate a stellar population of star-forming galaxies at z similar to 4 by focusing on the slope of their rest-frame ultraviolet (UV) continuum, beta, where f(lambda) proportional to lambda(beta). We investigate a sample of bright Lyman bre...
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 484(4) 5868-5887 2019年4月
In the SSA22 field which exhibits a large-scale proto-cluster at z = 3.1, we carried out a spectroscopic survey for Lyman Break Galaxies (LBGs) with the VLT/VIMOS and identified 78 confident LBGs at z = 2.5-4. We stacked their spectra in the obser...
Evan A. Rich   John P. Wisniewski   Thayne Currie   Misato Fukagawa   Carol A. Grady   Michael L. Sitko   Monika Pikhartova   Jun Hashimoto   Lyu Abe   Wolfgang Brandner   Timothy D. Brandt   Joseph C. Carson   Jeffrey Chilcote   Ruobing Dong   Markus Feldt   Miwa Goto   Tyler Groff   Olivier Guyon   Yutaka Hayano   Masahiko Hayashi   Saeko S. Hayashi   Thomas Henning   Klaus W. Hodapp   Miki Ishii   Masanori Iye   Markus Janson   Nemanja Jovanovic   Ryo Kandori   Jeremy Kasdin   Gillian R. Knapp   Tomoyuki Kudo   Nobuhiko Kusakabe   Masayuki Kuzuhara   Jungmi Kwon   Julien Lozi   Frantz Martinache   Taro Matsuo   Satoshi Mayama   Michael W. McElwain   Shoken Miyama   Jun-Ichi Morino   Amaya Moro-Martin   Takao Nakagawa   Tetsuo Nishimura   Tae-Soo Pyo   Eugene Serabyn   Hiroshi Suto   Ray W. Russel   Ryuji Suzuki   Michihiro Takami   Naruhisa Takato   Hiroshi Terada   Christian Thalmann   Edwin L. Turner   Taichi Uyama   Kevin R. Wagner   Makoto Watanabe   Toru Yamada   Hideki Takami   Tomonori Usuda   Motohide Tamura   
ASTROPHYSICAL JOURNAL 875(1) 2019年4月
We present H-band polarized scattered light imagery and JHK high-contrast spectroscopy of the protoplanetary disk around HD 163296 observed with the High-Contrast Coronographic Imager for Adaptive Optics (HiCIAO) and Subaru Coronagraphic Extreme A...
We report an orbital characterization of GJ1108Aab that is a low-mass binary system in the pre-main-sequence phase. Via the combination of astrometry using adaptive optics and radial velocity measurements, an eccentric orbital solution of e = 0.63...
P. R. Roelfsema   H. Shibai   L. Armus   D. Arrazola   M. Audard   M. D. Audley   C. M. Bradford   Charles, I   P. Dieleman   Y. Doi   L. Duband   M. Eggens   J. Evers   Funaki, I   J. R. Gao   M. Giard   A. di Giorgio   L. M. Gonzalez Fernandez   M. Griffin   F. P. Helmich   R. Hijmering   R. Huisman   D. Ishihara   N. Isobe   B. Jackson   H. Jacobs   W. Jellema   Kamp, I   H. Kaneda   M. Kawada   F. Kemper   F. Kerschbaum   P. Khosropanah   K. Kohno   P. P. Kooijman   O. Krause   J. van der Kuur   J. Kwon   W. M. Laauwen   G. de Lange   B. Larsson   D. van Loon   S. C. Madden   H. Matsuhara   F. Najarro   T. Nakagawa   D. Naylor   H. Ogawa   T. Onaka   S. Oyabu   A. Poglitsch   Reveret, V   L. Rodriguez   L. Spinoglio   Sakon, I   Y. Sato   K. Shinozaki   R. Shipman   H. Sugita   T. Suzuki   F. F. S. van der Tak   J. Torres Redondo   T. Wada   S. Y. Wang   C. K. Wafelbakker   H. van Weers   S. Withington   B. Vandenbussche   T. Yamada   Yamamura, I   
PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF AUSTRALIA 35 2018年8月
Measurements in the infrared wavelength domain allow direct assessment of the physical state and energy balance of cool matter in space, enabling the detailed study of the processes that govern the formation and evolution of stars and planetary sy...