Zobrazeno 1 - 10
of 103
pro vyhledávání: '"Toshinori Maihara"'
Autor:
Fumihide Iwamuro, Kazuya Matsubayashi, Mikio Kurita, Tetsuya Nagata, Keisuke Takahashi, Kazunari Shibata, Toshinori Maihara, Kouji Ohta, Kodai Yamamoto, Yoshikazu Nakatani, Michitoshi Yoshida, D. Kuroda, Ichiro Jikuya, Masatsugu Iribe, M. Kino, Daisaku Nogami, Hitoshi Tokoro, Hideyuki Izumiura, Hironori Tsutsui, Hiroshi Ohtani
Publikováno v:
Publications of the Astronomical Society of Japan. 72
An overview of the Seimei telescope, a 3.8 m optical infrared telescope located on Mt. Chikurinji in the Okayama prefecture of Japan, is presented. Seimei is a segmented-mirror telescope whose primary mirror consists of 18 petal-shaped segments. The
Autor:
Masahiko Kimura, Toshinori Maihara, Kouji Ohta, Fumihide Iwamuro, Sigeru Eto, Masafumi Lino, Daisaku Mochida, Takanori Shima, Hiroshi Karoji, Junichi Noumaru, Masayuki Akiyama, Jurek Brzeski, Peter R. Gillingham, Anna M. Moore, Greg Smith, Gavin B. Dalton, Ian A. Tosh, Graham J. Murray, David J. Robertson, Naoyuki Tamura
The Fibre Multi-Object Spectrograph (FMOS) is a second-generation common-use instrument of the Subaru telescope. Under an international collaboration scheme of Japan, UK, and Australia, a realistic design of FMOS has been already in completion, and t
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::607c1dc31bc4dce03b37386e2a197f7f
https://doi.org/10.1117/12.461208
https://doi.org/10.1117/12.461208
Autor:
Fumihide Iwamuro, Duncan Farrah, Michael Page, Naoyuki Tamura, V. Buat, Edward Macaulay, Isaac Roseboom, T. Mauch, James J. Bock, David L. Clements, Masayuki Akiyama, Caitlin M. Casey, Edward L. Chapin, M. Symeonidis, A. Cooray, Masanao Sumiyoshi, S. J. Oliver, Michael Zemcov, Kouji Ohta, Andrew Bunker, Toshinori Maihara, S. J. Ham, Emma Curtis-Lake, A. Conley, Douglas Scott, D. G. Bonfield, Masashi Kimura, Georgios E. Magdis, Y. Moritani, Ian Lewis, Gary Dalton, Naruhisa Takato, Edo Ibar, Bernhard Schulz, Tomonori Totani, J. S. Dunlop, Kiyoto Yabe, G. Marsden, Lian-Tao Wang
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 426:1782-1792
We investigate the properties (e.g. star formation rate, dust attentuation, stellar mass and metallicity) of a sample of infrared luminous galaxies at z \sim 1 via near-IR spectroscopy with Subaru-FMOS. Our sample consists of Herschel SPIRE and Spitz
Autor:
Gavin Dalton, Peter Gillingham, Masanao Sumiyoshi, Naoyuki Tamura, Junichi Noumaru, Alan R. Holmes, Yuuki Moritani, Scott Smedley, Roger Haynes, Brian Elms, Norio Ohshima, Fumihide Iwamuro, Graham J. Murray, Shigeru Eto, Nigel Dipper, Greg C. Smith, Philip J. Tait, Gabriella Frost, Guy F.W. Woodhouse, Masayuki Akiyama, Kouji Ohta, David J. Robertson, Tim R. Froud, Anna M. Moore, Daisaku Mochida, Masahiko Kimura, Rolf Müller, Kaori Kawate, Hanshin Lee, Emma Curtis Lake, Tony Farrell, Toshinori Maihara, Ray M. Sharples, D. G. Bonfield, Ian Lewis, Tomio Kurakami, Naruhisa Takato, Charles B. Brooks, Kiyoto Yabe, Ian Tosh, Colin Blackburn, Jurek Brzeski
Publikováno v:
Scopus-Elsevier
ResearcherID
ResearcherID
Fibre Multi-Object Spectrograph (FMOS) is the first near-infrared instrument with a wide field of view capable of acquiring spectra simultaneously from up to 400 objects. It has been developed as a common-use instrument for the F=2 prime-focus of the
Autor:
Surhud More, Takahiko Matsubara, Pedro G. Ferreira, Hiroyuki Okada, Tomonori Totani, István Szapudi, Gavin Dalton, Karl Glazebrook, Kouji Ohta, Motonari Tonegawa, Tomotsugu Goto, Takashi Ishikawa, Andrew Bunker, Kiyoto Yabe, Will J. Percival, Ikkoh Shimizu, Masayuki Akiyama, Teppei Okumura, Chiaki Hikage, Naruhisa Takato, Lee R. Spitler, Toshinori Maihara, Carlos S. Frenk, Naoyuki Tamura, Fumihide Iwamuro, Jean Coupon
Publikováno v:
Publications of the Astronomical Society of Japan, 2015, Vol.67(5), pp.81 [Peer Reviewed Journal]
FastSound is a galaxy redshift survey using the near-infrared Fiber Multi-Object Spectrograph (FMOS) mounted on the Subaru Telescope, targeting H$\alpha$ emitters at $z \sim 1.18$--$1.54$ down to the sensitivity limit of H$\alpha$ flux $\sim 2 \times
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d92339234ea719d0301e1bb34f98f2b8
http://dro.dur.ac.uk/18255/1/18255.pdf
http://dro.dur.ac.uk/18255/1/18255.pdf
Autor:
Norio Kaifu, Yumiko Oasa, Yoichi Itoh, Kentaro Motohara, Fumihiko Iwamuro, Toshinori Maihara, Saeko S. Hayashi, Masahiko Hayashi, Yasushi Nakajima, Motohide Tamura
Publikováno v:
The Astronomical Journal. 131:1608-1628
We present the results of deep near-infrared observations searching for very low mass young stellar objects (YSOs) in the massive star-forming region of S106 taken with the Subaru Telescope. The survey, whose limiting magnitude exceeds 20 mag in the
Autor:
Fumihide Iwamuro, Shinya Morita, Hitoshi Ohmori, Qing Liu, Toshinori Maihara, Shaohui Yin, Daisaku Mochida, Yoshihiro Uehara, Weimin Lin
Publikováno v:
International Journal of Machine Tools and Manufacture. 45:1598-1604
To explore various scientific frontiers from nearby substellar objects to large scale structures of the high redshift universe, a Fibre Multi-Object Spectrograph (FMOS) is being developed as the second generation near-infrared measuring instrument fo
Autor:
Yosuke Minowa, Yuzuru Yoshii, Tomonori Totani, Fumihide Iwamuro, Hideki Takami, Naruhisa Takato, Toshinori Maihara, Masanori Iye, Yutaka Hayano, Hiroshi Terada, Naoto Kobayashi, Shin Oya, Alan T. Tokunaga
Publikováno v:
The Astrophysical Journal. 629:29-44
We present a deep $K^{\prime}$-band (2.12$\mu$m) imaging of 1\arcmin\ $\times$ 1\arcmin Subaru Super Deep Field (SSDF) taken with the Subaru adaptive optics (AO) system. Total integration time of 26.8 hours results in the limiting magnitude of $K^{\p
Autor:
Fumihide Iwamuro, Yuzuru Yoshii, Toshinori Maihara, Kentaro Motohara, Masashi Kimura, Masao Doi, Shigeru Eto
Publikováno v:
The Astrophysical Journal. 614:69-74
Near-infrared spectra of four QSOs located at $z>6$ are obtained with the OH-airglow suppressor mounted on the Subaru telescope. The FeII/MgII emission-line ratios of these QSOs are examined by the same fitting algorithm as in our previous study of $
Publikováno v:
The Astrophysical Journal. 605:37-44
We describe observations of a galaxy in the field of the $z=2.483$ radio galaxy 4C 23.56, photometrically selected to have a spectral-energy distribution consistent with an old stellar population at the redshift of the radio galaxy. Exploration of re