Zobrazeno 1 - 10
of 35
pro vyhledávání: '"Daigo Tomono"'
Autor:
Katherine B. Follette, Gillian R. Knapp, Hideki Takami, Markus Janson, Amaya Moro-Martin, Yutaka Hayano, Sebastián Pérez, Eiji Akiyama, Shoken Miyama, Naruhisa Takato, Michael W. McElwain, Wolfgang Brandner, Takao Nakagawa, Thomas Henning, Masayuki Kuzuhara, Jerome de Leon, Edwin L. Turner, Satoshi Mayama, Tetsuo Nishimura, Takashi Tsukagoshi, Nemanja Jovanovic, Tomonori Usuda, Jeremy Kasdin, Miki Ishii, Thayne Currie, Tyler D. Groff, Nobuhiko Kusakabe, Hiroshi Terada, Evan A. Rich, Misato Fukagawa, Ryo Kandori, Daehyeon Oh, Michihiro Takami, Taichi Uyama, Takayuki Muto, Jun-Ichi Morino, John P. Wisniewski, Frantz Martinache, Taro Matsuo, Munetake Momose, Christian Thalmann, Carol A. Grady, Tomoyuki Kudo, Julien Lozi, Jun Hashimoto, Saeko S. Hayashi, Makoto Watanabe, Eugene Serabyn, Motohide Tamura, Markus Feldt, Miwa Goto, Masanori Iye, Masahiko Hayashi, Joseph C. Carson, Daigo Tomono, Hiroshi Suto, M. Bonnefoy, Tae-Soo Pyo, Olivier Guyon, Timothy D. Brandt, Toru Yamada, Ruobing Dong, Michael L. Sitko, Lyu Abe, Jeffrey Chilcote, Yi Yang, Klaus W. Hodapp, Ryuji Suzuki, Jungmi Kwon
Publikováno v:
The Astronomical Journal
The Astronomical Journal, American Astronomical Society, 2019, 159 (1), pp.12. ⟨10.3847/1538-3881/ab5850⟩
The Astronomical Journal, American Astronomical Society, 2019, 159 (1), pp.12. ⟨10.3847/1538-3881/ab5850⟩
The SR24 multi-star system hosts both circumprimary and circumsecondary disks, which are strongly misaligned from each other. The circumsecondary disk is circumbinary in nature. Interestingly, both disks are interacting, and they possibly rotate in o
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8570f3c7c413be000daf625206e270ce
Autor:
Masashi Chiba, Craig P. Loomis, Yoshihiko Yamada, Fumiaki Nakata, Yousuke Utsumi, Yutaka Komiyama, Toshifumi Futamase, Yao Cheng Lee, Yoshinori Miwa, Fumihiro Uraguchi, Paul T. P. Ho, Kyoji Nariai, Tomio Kurakami, Takashi Hamana, Yutaka Ezaki, Yoshiyuki Obuchi, Michael A. Strauss, Hideo Yokota, Dun Zen Jeng, Yukiko Kamata, Kazuyuki Kasumi, Satoru Iwamura, Eric J.-Y. Liaw, Naoki Yasuda, Hiroki Fujimori, Satoshi Kawanomoto, Hisanori Furusawa, Noboru Ito, Tadafumi Takata, Hisanori Suzuki, Atsushi J. Nishizawa, Chi Fang Chiu, Yusuke Hayashi, Robert Armstrong, Tomonori Usuda, Makoto Endo, Masamune Oguri, Hitomi Yamanoi, Hiroaki Aihara, Hitoshi Murayama, Robert H. Lupton, Kohei Imoto, Masaharu Muramatsu, Naoto Dojo, Michitaro Koike, Hiroyuki Ikeda, Kotaro Akutsu, Satoshi Miyazaki, Tomohisa Uchida, Satoshi Sofuku, James E. Gunn, Hiroshi Karoji, Masayuki Tanaka, Toru Matsuda, Masayuki Suzuki, Koei Yamamoto, Tomoaki Taniike, Daigo Tomono, Masahiro Takada, Edwin L. Turner, Kunio Takeshi, Yukie Oishi, Hironao Miyatake, Kazuhito Namikawa, H. Nakaya, Shoken Miyama, Tsang Chih Lai, Sogo Mineo, Norio Okada, Manobu M. Tanaka, Naoshi Sugiyama, Tsuyoshi Terai, James Bosch, Paul A. Price, Philip J. Tait, Shiang-Yu Wang, Yuki Okura, Yoshiyuki Doi, Hsin Yo Chen, Yoko Tanaka, Noboru Kawaguchi, Steve Bickerton, Tomoki Morokuma, Steward Smith, Cheng Lin Ho, Yasuhito Miyazaki
Publikováno v:
Publications of the Astronomical Society of Japan. 70
Autor:
Andreas Seltmann, Niranjan Thatte, Reiner Hofmann, Harald Weisz, Holger Mandel, Walter Seifert, Daigo Tomono
We present a system for the exchange and handling of cold field masks in LUCIFER, the near infrared camera and spectrograph for the LBT. Inside the LUCIFER cryostat, 10 field-stop and long-slit masks, and 23 multi-slit masks are stored in a stationar
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::69931ef8141628b0e6e7a7ab3fe4617d
https://ora.ox.ac.uk/objects/uuid:d2c032d5-a10d-47c0-a755-2ab6e9e8a237
https://ora.ox.ac.uk/objects/uuid:d2c032d5-a10d-47c0-a755-2ab6e9e8a237
Autor:
Jun Hashimoto, Amaya Moro-Martin, Masayuki Kuzuhara, Naruhisa Takato, Lyu Abe, Edwin L. Turner, Michihiro Takami, Yasuhiro H. Takahashi, Tetsuo Nishimura, Yutaka Hayano, Shoken Miyama, Takuya Suenaga, Ryuji Suzuki, Markus Janson, Tomonori Usuda, Tae-Soo Pyo, Michael W. McElwain, Joseph C. Carson, Olivier Guyon, Motohide Tamura, Toru Yamada, Hiroshi Terada, Christian Thalmann, Miki Ishii, C. Bergfors, Hiroshi Suto, Wolfgang Brandner, Hideki Takami, Bun'ei Sato, Tomoyuki Kudo, Taro Matsuo, Jun-Ichi Morino, Masahiko Hayashi, Ryo Kandori, Norio Narita, Eugene Serabyn, Thomas Henning, Taras Golota, Makiko Nagasawa, Miwa Goto, Klaus W. Hodapp, Shigeru Ida, Saeko S. Hayashi, Sebastian Egner, Makoto Watanabe, Markus Feldt, Gillian R. Knapp, Daigo Tomono, Nobuhiko Kusakabe
Publikováno v:
Publications of the Astronomical Society of Japan. 62(3):779-786
We present results of direct imaging observations for HAT-P-7 taken with the Subaru HiCIAO and the Calar Alto AstraLux. Since the close-in transiting planet HAT-P-7b was reported to have a highly tilted orbit, massive bodies such as giant planets, br
Autor:
Timothy D. Brandt, Tomonori Usuda, Joseph C. Carson, Nobuhiko Kusakabe, Christian Thalmann, Makoto Watanabe, Evan A. Rich, Daigo Tomono, Miki Ishii, Katherine B. Follette, Naruhisa Takato, Sebastian Egner, Lyu Abe, Chunhua Qi, Gillian R. Knapp, Michihiro Takami, Carol A. Grady, Amaya Moro-Martin, Thayne Currie, Takuya Suenaga, Miwa Goto, Yasuhiro H. Takahashi, Eiji Akiyama, Hiroshi Terada, Masayuki Kuzuhara, Michael W. McElwain, Jungmi Kwon, John P. Wisniewski, Tetsuo Nishimura, Thomas Henning, Eugene Serabyn, Tomoyuki Kudo, Jun-Ichi Morino, Catherine Espaillat, Ryuji Suzuki, Ryo Kandori, Shoken Miyama, Markus Feldt, Klaus W. Hodapp, Masanori Iye, Hideki Takami, Hiroshi Suto, Jun Hashimoto, Tae-Soo Pyo, Olivier Guyon, Edwin L. Turner, Motohide Tamura, Toru Yamada, Masahiko Hayashi, Saeko S. Hayashi, Wolfgang Brandner, Markus Janson, Yutaka Hayano, Satoshi Mayama, Taro Matsuo
We present the first spatially resolved polarized scattered light H-band detection of the DoAr 28 transitional disk. Our two epochs of imagery detect the scattered light disk from our effective inner working angle of 0.10" (13 AU) out to 0.50" (65 AU
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7b76704dbc82d4f8b110f16b75bf8270
http://arxiv.org/abs/1507.03014
http://arxiv.org/abs/1507.03014
Autor:
Masanori Iye, Thayne Currie, Masayuki Kuzuhara, Jeremy R. Swearingen, Eiji Akiyama, Tomoyuki Kudo, Timothy D. Brandt, Katherine B. Follette, Jun Hashimoto, Ray W. Russell, Gillian R. Knapp, Markus Feldt, Eugene Serabyn, Christian Thalmann, Nobuhiko Kusakabe, Lyu Abe, Wolfgang Brandner, Masahiko Hayashi, Michael W. McElwain, Takuya Suenaga, Jungmi Kwon, Makoto Watanabe, Ryuji Suzuki, Laird M. Close, Carol A. Grady, Marc J. Kuchner, Elizabeth H. Champney, Miwa Goto, Ryo Kandori, Joseph C. Carson, Michael L. Sitko, Daigo Tomono, Klaus W. Hodapp, Markus Janson, Satoshi Mayama, Tetsuo Nishimura, Miki Ishii, Thomas Henning, K. M. Maaskant, Misato Fukagawa, Shoken Miyama, Yutaka Hayano, Hiroshi Suto, Sebastian Egner, Amaya Moro-Martin, John P. Wisniewski, Naruhisa Takato, Taro Matsuo, Tomonori Usuda, Nienke van der Marel, Takayuki Muto, Edwin L. Turner, Motohide Tamura, Toru Yamada, Michiel Min, Tae-Soo Pyo, Hideki Takami, Olivier Guyon, Yasuhiro H. Takahashi, Hiroshi Terada, Jun-Ichi Morino, Michihiro Takami, Saeko S. Hayashi
Publikováno v:
The Astrophysical Journal, 798(2), 132
Astrophysical Journal, 798(2):132. IOP Publishing Ltd.
The Astrophysical Journal
Astrophysical Journal, 798(2):132. IOP Publishing Ltd.
The Astrophysical Journal
We present the first resolved near infrared imagery of the transition disk Oph IRS 48 (WLY 2-48), which was recently observed with ALMA to have a strongly asymmetric sub-millimeter flux distribution. H-band polarized intensity images show a $\sim$60A
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5dfd45d35efd937efe0cf820f4964fe6
http://adsabs.harvard.edu/abs/2015ApJ...798..132F
http://adsabs.harvard.edu/abs/2015ApJ...798..132F
Autor:
Ryo Kandori, Yasuhiro H. Takahashi, Hiroshi Terada, Klaus W. Hodapp, Hideki Takami, Thayne Currie, Ryuji Suzuki, Timothy D. Brandt, Wolfgang Brandner, Nobuhiko Kusakabe, Shoken Miyama, Takuya Suenaga, Eugene Serabyn, Markus Janson, Tomoyuki Kudo, Yoichi Itoh, Masayuki Kuzuhara, Yutaka Hayano, Michael W. McElwain, Jungmi Kwon, Naruhisa Takato, Hiroshi Suto, Gillian R. Knapp, Tetsuo Nishimura, Carol A. Grady, Satoshi Mayama, Taro Matsuo, Joseph C. Carson, Thomas Henning, Masahiko Hayashi, Sebastian Egner, Makoto Watanabe, Miki Ishii, Lyu Abe, Yumiko Oasa, Daigo Tomono, Edwin L. Turner, Markus Feldt, Motohide Tamura, Toru Yamada, Christian Thalmann, Tae-Soo Pyo, Olivier Guyon, Jun Hashimoto, Amaya Moro-Martin, Saeko S. Hayashi, Masanori Iye, Jun-Ichi Morino, Tomonori Usuda, John P. Wisniewski
A high angular resolution near-infrared polarized-intensity image of the GG Tau A binary system was obtained with the Subaru Telescope. The image shows the circumbinary disk scattering the light from the central binary. The azimuthal profile of the p
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::53b8a6f87a1e8f05d1f092cae4042095
Autor:
Masanori Iye, Carol A. Grady, Makoto Watanabe, Miwa Goto, Eiji Akiyama, Masayuki Kuzuhara, Tomoyuki Kudo, Jun-Ichi Morino, Thayne Currie, Ryo Kandori, Markus Feldt, Daigo Tomono, Katherine B. Follette, Naruhisa Takato, Lyu Abe, Michael L. Sitko, Michael W. McElwain, Jungmi Kwon, Klaus W. Hodapp, Hiroshi Suto, Tetsuo Nishimura, N. Kusakabe, Gillian R. Knapp, Jerome de Leon, Satoshi Mayama, Masahiko Hayashi, Yutaka Hayano, Michihiro Takami, Christian Thalmann, Saeko S. Hayashi, Ryuji Suzuki, Taro Matsuo, Tae-Soo Pyo, Olivier Guyon, Yasuhiro H. Takahashi, Timothy D. Brandt, Hiroshi Terada, Joseph C. Carson, Takuya Suenaga, John P. Wisniewski, Thomas Henning, Hideki Takami, Hauyu Baobab Liu, Wolfgang Brandner, Miki Ishii, Sebastian Egner, Tomonori Usuda, Edwin L. Turner, Shoken Miyama, Motohide Tamura, Markus Janson, Toru Yamada, Jennifer L. Karr, Eugene Serabyn, Jun Hashimoto, Amaya Moro-Martin
We present new high-resolution ($\sim$0\farcs09) $H$-band imaging observations of the circumstellar disk around the T Tauri star SU Aur. Our observations with Subaru-HiCIAO have revealed the presence of scattered light as close as 0\farcs15 ($\sim$20
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ec21d38c568f8b14e1d472285ee15152
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
Autor:
Makoto Watanabe, Tomoyuki Kudo, Masayuki Kuzuhara, Yutaka Hayano, Markus Feldt, Daigo Tomono, Ruobing Dong, John P. Wisniewski, Timothy D. Brandt, Mitsuhiko Honda, Michael W. McElwain, Jungmi Kwon, Ryuji Suzuki, Tomonori Usuda, Jun-Ichi Morino, Thomas Henning, Michael L. Sitko, Satoshi Mayama, Pin-Gao Gu, Sebastian Egner, Thayne Currie, Katherine B. Follette, Edwige Chapillon, Tetsuo Nishimura, Youchi Itoh, Eugene Serabyn, Gillian R. Knapp, Jennifer L. Karr, Markus Janson, Taro Matsuo, Joseph C. Carson, Ryo Kandori, Hideki Takami, Christian Thalmann, Klaus W. Hodapp, Miki Ishii, Eiji Akiyama, Naruhisa Takato, Masanori Iye, Saeko S. Hayashi, Carol A. Grady, Tae-Soo Pyo, Olivier Guyon, Wolfgang Brandner, N. Kusakabe, Ya-Wen Tang, Hiroshi Suto, Takayuki Muto, Edwin L. Turner, Motohide Tamura, Toru Yamada, Lyu Abe, Masahiko Hayashi, Yasuhiro Hasegawa, Shoken Miyama, Michihiro Takami, Yasuhiro H. Takahashi, Hiroshi Terada, Amaya Moro-Martin, Takuya Suenaga, Jun Hashimoto
We present a new method of analysis for determining the surface geometry of five protoplanetary disks observed with near-infrared imaging polarimetry using Subaru-HiCIAO. Using as inputs the observed distribution of polarized intensity (PI), disk inc
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b466aab6fdd93c09794ade008a04eaa3