Zobrazeno 1 - 10
of 97
pro vyhledávání: '"Sato, Taro"'
Publikováno v:
In Building and Environment January 2023 227 Part 2
Autor:
Shimozaki, Keitaro, Hirata, Kenro, Sato, Taro, Nakamura, Maho, Kato, Kyoko, Hirano, Hidekazu, Kumekawa, Yosuke, Hino, Kaori, Kawakami, Kentaro, Kito, Yosuke, Matsumoto, Toshihiko, Kawakami, Takeshi, Komoda, Masato, Nagashima, Kengo, Sato, Yasunori, Yamazaki, Kentaro, Hironaka, Shuichi, Takaishi, Hiromasa, Hamamoto, Yasuo, Muro, Kei
Publikováno v:
In Clinical Colorectal Cancer December 2022 21(4):339-346
Autor:
Sarkar, Avijite Kumer, Nakamura, Shiro, Nakai, Kento, Sato, Taro, Shiga, Takahiro, Abe, Yuka, Hoashi, Yurie, Inoue, Tomio, Akamatsu, Wado, Baba, Kazuyoshi
Publikováno v:
In Stem Cell Research March 2022 59
Akademický článek
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Autor:
Nakayama, Izuma, Takahari, Daisuke, Wakatsuki, Takeru, Osumi, Hiroki, Chin, Keisho, Ogura, Mariko, Sato, Taro, Suzuki, Takeshi, Kamiimabeppu, Daisaku, Ooki, Akira, Suenaga, Mitsukuni, Shinozaki, Eiji, Yamaguchi, Kensei
Publikováno v:
In ESMO Open 2020 5(2)
We study the angular clustering of z~2 galaxies using ~40,000 star-forming (SF) and ~5,000 passively-evolving (PE) galaxies selected from ~2.5 deg$^2$ of deep ($K_{lim}$=23-24 AB) CFHT imaging. For both populations the clustering is stronger for gala
Externí odkaz:
http://arxiv.org/abs/1407.2319
We investigate the luminosity dependent clustering of rest-frame UV selected galaxies at z~4, 3, 2.2, and 1.7 in the Keck Deep Fields (KDFs), which are complete to R = 27 and cover 169 arcmin^2. We find that at z~4 and 3, UV-bright galaxies cluster m
Externí odkaz:
http://arxiv.org/abs/1106.2146
Publikováno v:
Astrophys.J.696:214-232,2009
We report on a S/N-limited search for low-ionization gas outflows in the spectra of the 0.11 < z < 0.54 objects in the EGS portion of the DEEP2 survey. Doppler shifts from the host galaxy redshifts are systematically searched for in the Na I 5890,96
Externí odkaz:
http://arxiv.org/abs/0804.4312
Infalling Faint [OII] Emitters in Abell 851. II. Environment, Kinematics, and Star Formation History
Autor:
Sato, Taro, Martin, Crystal L.
Publikováno v:
Astrophys.J.647:946-969,2006
We report on the environments, kinematics, and SFH of [OII]-selected objects in the z=0.4 galaxy cluster A851, using Keck optical spectra. A large fraction (~55%) of cluster [OII] emitters show strong Balmer absorptions (>4A in equivalent width at Hd
Externí odkaz:
http://arxiv.org/abs/astro-ph/0605044
Autor:
Sato, Taro, Martin, Crystal L.
Publikováno v:
Astrophys.J.647:934-945,2006
We report on a spectroscopic confirmation of narrowband-selected [OII] emitters in Abell 851 catalogued by Martin et al. (2000). The optical spectra obtained from the Keck I Low Resolution Imaging Spectrometer (LRIS) and Keck II Deep Imaging Multi-Ob
Externí odkaz:
http://arxiv.org/abs/astro-ph/0605043