Naoto Kobayashi
University of Tokyo
229 Papers
1.4K Citations
Naoto Kobayashi is an academic researcher from University of Tokyo. The author has contributed to research in topics: Galaxy & Star formation. The author has an hindex of 38, co-authored 228 publications. Previous affiliations of Naoto Kobayashi include Kyoto Sangyo University & Subaru.
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Papers
Structural studies of eight bright rimmed clouds in the southern hemisphere
Saurabh Sharma,Ashwani Pandey,Jura Borissova,Jura Borissova,Devendra K. Ojha,Valentin D. Ivanov,Katsuo Ogura,Naoto Kobayashi,Radostin Kurtev,Radostin Kurtev,M. Gopinathan,Ram Kesh Yadav +11 more
TL;DR: In this article, the authors carried out deep and wide-field near and mid-infrared observations for a sample of eight bright-rimmed clouds (BRCs) supplemented with the Spitzer archival data, and extracted 13 stellar cores of eight or more members, which contain 60% of the total YSOs.
The Tomo-e Gozen wide field CMOS camera for the Kiso Schmidt telescope
Shigeyuki Sako,Ryou Ohsawa,Hidenori Takahashi,Yuto Kojima,Mamoru Doi,Naoto Kobayashi,Tsutomu Aoki,Noriaki Arima,Ko Arimatsu,Makoto Ichiki,Shiro Ikeda,Kota Inooka,Yoshifusa Ita,Toshihiro Kasuga,Mitsuru Kokubo,Masahiro Konishi,Hiroyuki Maehara,Noriyuki Matsunaga,Kazuma Mitsuda,Takashi Miyata,Yuki Mori,Mikio Morii,Tomoki Morokuma,Kentaro Motohara,Yoshikazu Nakada,Shin-ichiro Okumura,Yuki Sarugaku,Mikiya Sato,Toshikazu Shigeyama,Takao Soyano,Masaomi Tanaka,Ken'ichi Tarusawa,Nozomu Tominaga,Tomonori Totani,Seitaro Urakawa,Fumihiko Usui,Jun-ichi Watanabe,Takuya Yamashita,Makoto Yoshikawa +38 more
- 06 Jul 2018
TL;DR: The Tomo-e Gozen camera as discussed by the authors is a high-speed camera for the Kiso 10m Schmidt telescope with a field-of-view of 207-deg2 covered by 84 chips of 2k x 1k CMOS image sensors with 19μm pixels.
Down‐sizing in galaxy formation at z∼ 1 in the Subaru/XMM–Newton Deep Survey (SXDS)
Tadayuki Kodama,Toru Yamada,Masayuki Akiyama,Kentaro Aoki,Mamoru Doi,Hisanori Furusawa,Tetsuharu Fuse,Masatoshi Imanishi,Cathy Ishida,Masanori Iye,Masaru Kajisawa,Hiroshi Karoji,Naoto Kobayashi,Yutaka Komiyama,George Kosugi,Yoshitomo Maeda,Satoshi Miyazaki,Yoshihiko Mizumoto,Tomoki Morokuma,Fumiaki Nakata,Junichi Noumaru,Ryusuke Ogasawara,Masami Ouchi,Toshiyuki Sasaki,Kazuhiro Sekiguchi,Kazuhiro Shimasaku,Chris Simpson,Tadafumi Takata,Ichi Tanaka,Yoshihiro Ueda,Naoki Yasuda,Michitoshi Yoshida +31 more
TL;DR: In this article, the authors used the deep wide field optical imaging data of the Subaru/XMM-Newton Deep Survey to discuss the luminosity-dependent galaxy colours down to z = 25.2, corresponding to ∼M ∗ + 2( ∼ 10 10 M� with respect to passively evolving galaxies at z ∼ 1.
Adaptive Optics Rest-Frame V-Band Imaging of Lyman Break Galaxies at z~3: High Surface Density Disklike Galaxies?*
TL;DR: In this paper, the AO-assisted K-band imaging observations of z ~ 3 LBGs whose absolute magnitudes range from MV* − 0.5 mag to MV* + 3.0 mag were conducted to reveal the rest-frame V-band morphology of galaxies at z = 3.
Imaging and Spatially Resolved Spectroscopy of AFGL 2688 in the Thermal Infrared Region
TL;DR: In this paper, the authors presented ground-based high-resolution (0.3) imaging of AFGL 2688 at L' (3.8 um) and M'(4.7um).