Zobrazeno 1 - 10
of 76
pro vyhledávání: '"Shoken M. Miyama"'
Autor:
Tae-Soo Pyo, Tomoyuki Kudo, Julien Lozi, Olivier Guyon, Ryuji Suzuki, Jungmi Kwon, Masanori Iye, Joseph C. Carson, Hiroshi Suto, Jeffrey Chilcote, Masahiko Hayashi, Takao Nakagawa, Nemanja Jovanovic, Thomas Henning, Christian Thalmann, M. Bonnefoy, Yutaka Hayano, Tetsuo Nishimura, Eugene Serabyn, Miki Ishii, Klaus W. Hodapp, Yang Yang, Tomonori Usuda, Ryo Kandori, Michael W. McElwain, Makoto Watanabe, Eiji Akiyama, Toru Yamada, Taichi Uyama, Masayuki Kuzuhara, Gillian R. Knapp, Nobuhiko Kusakabe, Evan A. Rich, Shoken M. Miyama, Markus Janson, Carol A. Grady, Saeko S. Hayashi, Wolfgang Brandner, Lyu Abe, Jun-Ichi Morino, Jun Hashimoto, Michihiro Takami, Thayne Currie, Timothy D. Brandt, Motohide Tamura, Markus Feldt, Miwa Goto, Naruhisa Takato, Jeremy Kasdin, Tyler D. Groff, Hideki Takami, Edwin L. Turner, John P. Wisniewski, Frantz Martinache, Satoshi Mayama, Ruobing Dong, Hiroshi Terada, Amaya Moro-Martin, Taro Matsuo
Publikováno v:
The Astrophysical Journal
The Astrophysical Journal, 2020, 889 (2), pp.140. ⟨10.3847/1538-4357/ab64f9⟩
The Astrophysical Journal, American Astronomical Society, 2020, 889 (2), pp.140. ⟨10.3847/1538-4357/ab64f9⟩
The Astrophysical Journal, 2020, 889 (2), pp.140. ⟨10.3847/1538-4357/ab64f9⟩
The Astrophysical Journal, American Astronomical Society, 2020, 889 (2), pp.140. ⟨10.3847/1538-4357/ab64f9⟩
We analyzed the young (2.8-Myr-old) binary system FS Tau A using near-infrared (H-band) high-contrast polarimetry data from Subaru/HiCIAO and sub-millimeter CO (J=2-1) line emission data from ALMA. Both the near-infrared and sub-millimeter observatio
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::bf6155ecb6ef252be3d014e246d38a64
https://hal.science/hal-03518334/document
https://hal.science/hal-03518334/document
Autor:
Tomoyuki Kudo, Thomas Henning, Mickael Bonnefoy, Michael W. McElwain, Makoto Watanabe, Yutaka Hayano, Timothy D. Brandt, Sebastian Egner, Amaya Moro-Martin, Christian Thalmann, Takayuki Muto, Eugene Serabyn, Edwin L. Turner, Ryuji Suzuki, Carol A. Grady, Itsuki Sakon, Satoshi Mayama, Yasuhiro H. Takahashi, Markus Janson, Shoken M. Miyama, Klaus W. Hodapp, Hideki Takami, Tetsuo Nishimura, Toru Yamada, Thayne Currie, Masahiko Hayashi, John P. Wisniewski, Miki Ishii, Naruhisa Takato, Taro Matsuo, Saeko S. Hayashi, Tae-Soo Pyo, Nobuhiko Kusakabe, Takuya Suenaga, Jeffrey Fung, Yang Yang, Olivier Guyon, Michihiro Takami, Lyu Abe, Markus Feldt, Miwa Goto, Taichi Uyama, Tomonori Usuda, Jun-Ichi Morino, Eiji Akiyama, Ryo Kandori, Jun Hashimoto, Jungmi Kwon, Wolfgang Brandner, Masanori Iye, Joseph C. Carson, Motohide Tamura, Hiroshi Terada, Jerome de Leon, Hiroshi Suto, Ruobing Dong, Michael L. Sitko, Masayuki Kuzuhara, Gillian R. Knapp
Publikováno v:
The Astronomical Journal. 156(2)
著者人数: 59名（所属. 宇宙航空研究開発機構宇宙科学研究所(JAXA)(ISAS): 權, 靜美)
Accepted: 2018-06-08
資料番号: SA1180097000
Accepted: 2018-06-08
資料番号: SA1180097000
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0c96c7b1a5a28d2bd1be9c60a34ad1bd
http://id.nii.ac.jp/1696/00029868/
http://id.nii.ac.jp/1696/00029868/
Autor:
Saeko S. Hayashi, Takayuki Muto, M. Feldt, Miwa Goto, Jennifer I-Hsiu Li, Tetsuo Nishimura, Hideki Takami, Th. Henning, Motohide Tamura, Ryo Kandori, Takuya Suenaga, Yutaka Hayano, M. L. Sitko, Hiroshi Terada, Tetsuo Taki, M. Bonnefoy, M. Hayashi, Hauyu Baobabu Liu, Nagayoshi Ohashi, Shoken M. Miyama, Gillian R. Knapp, M. W. McElwain, Sebastian Egner, Ruobing Dong, Tomonori Usuda, Timothy D. Brandt, Tae-Soo Pyo, Eugene Serabyn, Olivier Guyon, Tomoyuki Kudo, Makoto Watanabe, John P. Wisniewski, Eiji Akiyama, Taro Matsuo, D. Tomono, Markus Janson, Miki Ishii, T. Tsukagoshi, Munetake Momose, C. A. Grady, Masayuki Kuzuhara, Wolfgang Brandner, Amaya Moro-Martin, Yasuhiro Hasegawa, Lyu Abe, Jungmi Kwon, Masanori Iye, Joseph C. Carson, Klaus W. Hodapp, Hiroshi Suto, Edwin L. Turner, Y. H. Takahashi, Jun-Ichi Morino, Jun Hashimoto, Satoshi Mayama, N. Kusakabe, Naruhisa Takato, C. Thalmann, Michihiro Takami, R. Suzuki, Toru Yamada
Publikováno v:
NASA Astrophysics Data System
Dust trapping accelerates the coagulation of dust particles, and thus it represents an initial step toward the formation of planetesimals. We report $H$-band (1.6 um) linear polarimetric observations and 0.87 mm interferometric continuum observations
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::06f8b6dfe5194df63590ee43a28f8f7e
http://arxiv.org/abs/1607.04708
http://arxiv.org/abs/1607.04708
Autor:
Shin Oya, Norio Kaifu, Masahiko Hayashi, Takayuki Nishikawa, Hiroyasu Ando, Saeko S. Hayashi, Yoichi Itoh, Misato Fukagawa, Satoshi Mayama, Takuya Yamashita, Jun-Ichi Morino, Hiroshi Suto, Miki Ishii, Motohide Tamura, Tomoyuki Kudo, Tae-Soo Pyo, T. Naoi, Tomonori Usuda, Shoken M. Miyama, K. Murakawa, Yumiko Oasa
Publikováno v:
Publications of the Astronomical Society of Japan. 58(2):375-382
High angular resolution near-infrared (JHK) adaptive optics images of T Tau were obtained with the infrared camera Coronagraphic Imager with Adaptive Optics (CIAO) mounted on the 8.2m Subaru Telescope in 2002 and 2004. The images resolve a complex ci
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d97276856e1fc1911b3822171973db55
https://hdl.handle.net/20.500.14094/90001433
https://hdl.handle.net/20.500.14094/90001433
Autor:
Jun-Ichi Morino, Yoichi Itoh, B. R. Oppenheimer, Takashi Tsuji, Koji Murakawa, Tadashi Nakajima, Shin Oya, Shoken M. Miyama, Hiroshi Suto, Miki Ishii, Motohide Tamura, Naruhisa Takato, Yumiko Oasa, Saeko S. Hayashi, Hideki Takami, Tomoyuki Kudo, Misato Fukagawa
Publikováno v:
Astronomische Nachrichten. 326:952-957
We have started a corongraphic search for brown dwarfs and planets around young nearby stars within 20 pc of the Sun, using the adaptive optics coronagraph, CIAO, on Subaru. The dynamic range we have achieved is ΔK = 13 at 2.5″ from the central st
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::4c169ab5da4db35b52b553cfc86c238d
https://doi.org/10.1002/asna.200510445
https://doi.org/10.1002/asna.200510445
Autor:
Akitoshi Ueda, Takashi Nakamura, Nobuki Kawashima, Masaki Ando, Shigeo Nagano, Ken'ichi Nakagawa, Koji Arai, Kozo Ueda, Norihiko Kamikubota, Masatake Ohashi, Akito Araya, Daisuke Tatsumi, Eiichi Mizuno, Nobuyuki Kanda, Atsushi Sekiya, Shigenori Moriwaki, Shinji Miyoki, Kuniharu Tochikubo, Mitsuru Musha, Ryutaro Takahashi, Takahiro Tanaka, Ken-ichi Ueda, Norikatsu Mio, Sumihiro Matsumura, Kazuaki Kuroda, N. Ohishi, Shuichi Sato, Misao Sasaki, Shoken M. Miyama, M. A. Barton, Nobuhiro Tsuda, Toshitaka Yamazaki, Hideki Ishizuka, Koichi Waseda, Takayuki Tomaru, Hideki Asada, Ken-ichi Oohara, Masaru Shibata, Osamu Miyakawa, Gen'ichi Horikoshi, Yujiro Ogawa, Akiteru Takamori, Kazuhiro Yamamoto, Yoshihide Kozai, Hideyuki Tagoshi, Shigemi Otsuka, Mitsuhiro Fukushima, Toshikazu Suzuki, Yasufumi Kojima, Keita Kawabe, Toshifumi Futamase, Ken-ichi Nakao, Shinsuke Taniguchi, Namio Matsuda, Seiji Kawamura, Takashi Uchiyama, Masa-Katsu Fujimoto, Kimio Tsubono, Yoshio Saito, Souichi Telada
Publikováno v:
Review of Scientific Instruments. 74:4176-4183
Laser frequency stabilization is essential for interferometric gravitational-wave detectors to attain their target sensitivity. We have designed a multistage laser frequency stabilization system which has been applied in the development of the TAMA 3
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::176ebaf4f50323c86ef522a9cb6fe210
https://doi.org/10.1063/1.1597958
https://doi.org/10.1063/1.1597958
Publikováno v:
Astrophysics and Space Science. 284:739-742
We have tested the applicability of the global modal approach in the density wave theory of spiral structure for a sample of spiral galaxies with measured axisymmetric background properties. We report here the results of the simulations for four gala
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::ad5955350bdf23a63927ad78e4036fd6
https://doi.org/10.1023/a:1024040331638
https://doi.org/10.1023/a:1024040331638
Autor:
Akito Araya, Hideki Ishizuka, Mitsuru Musha, Takahiro Tanaka, Akitoshi Ueda, Namio Matsuda, Mitsuhiro Fukushima, K. Oohara, Nobuki Kawashima, Daisuke Tatsumi, Shigeo Nagano, Shinji Miyoki, Koji Arai, Seiji Kawamura, Takashi Nakamura, Gen'ichi Horikoshi, Kuniharu Tochikubo, Masaki Ando, Nobuhiro Tsuda, Kazuaki Kuroda, Masa Katsu Fujimoto, Nobuyuki Kanda, Misao Sasaki, Norihiko Kamikubota, M. A. Barton, Takayuki Tomaru, Toshikazu Suzuki, Masatake Ohashi, Takashi Uchiyama, Kimio Tsubono, Yoshio Saito, Shigenori Moriwaki, Yasufumi Kojima, Yujiro Ogawa, Akiteru Takamori, Kazuhiro Yamamoto, N. Ohishi, Ken-ichi Ueda, Souichi Telada, Ken'ichi Nakagawa, Ryutaro Takahashi, Sumihiro Matsumura, Osamu Miyakawa, Keita Kawabe, Yoshihide Kozai, Hideyuki Tagoshi, Toshitaka Yamazaki, Toshifumi Futamase, Eiichi Mizuno, Norikatsu Mio, Shinsuke Taniguchi, Shuichi Sato, Shoken M. Miyama
Publikováno v:
Review of Scientific Instruments. 73:2136-2142
We have developed a light source suitable for laser interferometric gravitational-wave detectors. The developed light source has high power, TEM00 mode, linear polarization, high frequency stability, and low intensity noise. The light source with the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::ee38aafa40009ca39c308baac16714dd
https://doi.org/10.1063/1.1470230
https://doi.org/10.1063/1.1470230
Autor:
Eiji Kambe, Yoichi Takeda, Shoken M. Miyama, S. Wada, Seiji Masuda, Hideyuki Izumiura, Yuji Norimoto, Fumihiro Uraguchi, Hiroyasu Ando, Hideo Maehara, Satoshi Kawanomoto, Kenshi Yanagisawa, Hisashi Koyano, B. Sato, Norio Okada, Hideaki Miyazaki, Etsuji Watanabe, Takafumi Okada, Yasuhiro Shimizu, Michitoshi Yoshida
Publikováno v:
Publications of the Astronomical Society of Japan. 54:113-120
Toward the aims of spectroscopically searching for planetary systems around stars, or detecting oscillations of solar-type stars for stellar seismology, we have started an experimental project of very precise determinations of stellar radial velocity
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::01336a6f81441b2f4a390291c664c861
https://doi.org/10.1093/pasj/54.1.113
https://doi.org/10.1093/pasj/54.1.113
Autor:
Nobuhiko Kusakabe, Amaya Moro-Martin, Takuya Suenaga, Motohide Tamura, Jungmi Kwon, Tetsuo Nishimura, Jun-Ichi Morino, Jun Hashimoto, Christian Thalmann, Masahiko Hayashi, Takahiro Sumi, Thomas Henning, Tomoyuki Kudo, Tae-Soo Pyo, Masaru Kajisawa, Yutaka Hayano, Thayne Currie, Jun Sudo, Tomonori Usuda, Olivier Guyon, Hiroshi Shibai, Hideki Takami, Klaus W. Hodapp, Naruhisa Takato, Masayuki Kuzuhara, Lyu Abe, Wolfgang Brandner, Ryo Kandori, Miki Ishii, Nobuo Arimoto, Gillian R. Knapp, Timothy D. Brandt, Edwin L. Turner, Eugene Serabyn, Shoken M. Miyama, Carol A. Grady, Markus Janson, Michael W. McElwain, John P. Wisniewski, Sebastian Egner, Yasuhiro H. Takahashi, Yoichi Itoh, Saeko S. Hayashi, Makoto Watanabe, Masanori Iye, M. Samland, Joseph C. Carson, Markus Feldt, Miwa Goto, Daigo Tomono, Hiroshi Suto, Kodai Yamamoto, Ryuji Suzuki, Toru Yamada, Misato Fukagawa, Hiroshi Terada, Mihoko Konishi, Taro Matsuo
We compared the number of faint stars detected in deep survey fields with the current stellar distribution model of the Galaxy and found that the detected number in the H band is significantly smaller than the predicted number. This indicates that M-
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4a45ac17630adbca9a8e26a5710782c1