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Featured researches published by Masatoshi Imanishi.


Publications of the Astronomical Society of Japan | 2002

CISCO: Cooled Infrared Spectrograph and Camera for OHS on the Subaru Telescope

Kentaro Motohara; Fumihide Iwamuro; Toshinori Maihara; Shin Oya; Hiroyuki Tsukamoto; Masatoshi Imanishi; Hiroshi Terada; Miwa Goto; Jun Ichi Iwai; Hirohisa Tanabe; Ryuji Hata; Tomoyuki Taguchi; Takashi Harashima

This paper describes a Cooled Infrared Spectrograph and Camera for OHS (CISCO), mounted on the Nasmyth focus of the Subaru telescope. It is primarily designed as a back-end camera of the OH-Airglow Suppressor (OHS), and is also used as an independent, general-purpose near-infrared camera/spectrograph. CISCO is based on a single 1024x1024 format HgCdTe HAWAII array detector, and is capable of either wide-field imaging of 1.8x1.8 field-of-view or low-resolution spectroscopy from 0.9 to 2.4 um. The limiting magnitudes measured during test observations were found to be J=23.5mag and K=22.4mag (imaging, 1 aperture, S/N=5, 1 hr exposure).


Astronomical Telescopes and Instrumentation | 1998

CISCO: cooled infrared spectrograph and camera for OHS

Kentaro Motohara; Toshinori Maihara; Fumihide Iwamuro; Shin Oya; Masatoshi Imanishi; Hiroshi Terada; Miwa Goto; Jun Ichi Iwai; Hirohisa Tanabe; Hiroyuki Tuskamoto; Kazuhiro Sekiguchi

CISCO is an IR camera and spectrograph based on a single 1024 X 1024 HgCdTe array detector, which has been developed as a back-end spectrograph of OHS. It is also designed to be mounted on the Cassegrain or Nasmyth focus directly as an independent instrument. In addition to the normal imaging and spectroscopy modes, CISCO has a slitless prism spectroscopy mode at resolving power of approximately 30. This mode is primarily aimed at detecting the H(alpha) emission line of forming galaxy at z equals 2.05-2.65. The development of CISCO is in near completion, showing results of test observations carried out using a 1.5m telescope.


Publications of the Astronomical Society of Japan | 2000

Subaru Observations for the K-Band Luminosity Distribution of Galaxies in Clusters near to 3C 324 at z ∼ 1.2

Masaru Kajisawa; Toru Yamada; Ichi Tanaka; Toshinori Maihara; Fumihide Iwamuro; Hiroshi Terada; Miwa Goto; Kentaro Motohara; Hirohisa Tanabe; Tomoyuki Taguchi; Ryuji Hata; Masanori Iye; Masatoshi Imanishi; Yoshihiro Chikada; Chris Simpson; Toshiyuki Sasaki; George Kosugi; Tomonori Usuda; Tomio Kanzawa; Tomio Kurakami

We investigate the


Publications of the Astronomical Society of Japan | 2000

Infrared Imaging of the Gravitational Lens PG 1115+080 with the Subaru Telescope

Fumihide Iwamuro; Kentaro Motohara; Toshinori Maihara; Jun'ichi Iwai; Hirohisa Tanabe; Tomoyuki Taguchi; Ryuji Hata; Hiroshi Terada; Miwa Goto; Shin Oya; Masayuki Akiyama; Hiroyasu Ando; T. Aoki; Yoshihiro Chikada; Mamoru Doi; Takeo Fukuda; Masaru Hamabe; Masahiko Hayashi; Saeko S. Hayashi; Toshihiro Horaguchi; Shin-ichi Ichikawa; Takashi Ichikawa; Masatoshi Imanishi; Katsumi Imi; Motoko Inata; Shuzo Isobe; Yoichi Itoh; Masanori Iye; Norio Kaifu; Yukiko Kamata

K


Publications of the Astronomical Society of Japan | 2000

High-Resolution Near-Infrared Imaging of the Powerful Radio Galaxy 3C 324 at z = 1.21 with the Subaru Telescope

Toru Yamada; Masaru Kajisawa; Ichi Tanaka; Toshinori Maihara; Fumihide Iwamuro; Hiroshi Terada; Miwa Goto; Kentaro Motohara; Hirohisa Tanabe; Tomoyuki Taguchi; Ryuji Hata; Masanori Iye; Masatoshi Imanishi; Yoshihiro Chikada; Michitoshi Yoshida; Chris Simpson; Toshiyuki Sakaki; George Kosugi; Tomonori Usuda; Koji Omata; Katsumi Imi

-band luminosity distribution of galaxies in the region of clusters at


Astronomical Telescopes and Instrumentation | 1998

LEWIS: a cross-dispersed spectrograph for the 3-μm region

Masatoshi Imanishi; Hiroshi Terada; Miwa Goto; Toshinori Maihara

zsim1.2


Publications of the Astronomical Society of Japan | 2000

The First Light of the Subaru Telescope: A New Infrared Image of the Orion Nebula

Norio Kaifu; Tomonori Usuda; Saeko S. Hayashi; Yoichi Itoh; Masayuki Akiyama; Takuya Yamashita; Yasushi Nakajima; Motohide Tamura; Shu-ichiro Inutsuka; Masahiko Hayashi; Toshinori Maihara; Fumihide Iwamuro; Kentaro Motohara; Jun'ich Iwai; Hirohisa Tanabe; Tomoyuki Taguchi; Ryuji Hata; Hiroshi Terada; Miwa Goto; Hiroyasu Ando; T. Aoki; Yoshihiro Chikada; Mamoru Doi; Noboru Ebizuka; Takeo Fukuda; Masaru Hamabe; Tetsuo Hasegawa; Toshihiro Horaguchi; Shin-ichi Ichikawa; Takashi Ichikawa

near to the radio galaxy 3C 324. The imaging data were obtained during the commissioning period of the Subaru telescope. There is a significant excess of the surface number density of the galaxies with


Publications of the Astronomical Society of Japan | 1997

Spectroscopic Study of NGC 1068 in the 3 μm Band

Masatoshi Imanishi; Hiroshi Terada; Kouji Sugiyama; Kentaro Motohara; Miwa Goto; Toshinori Maihara

K =


The Astronomical Journal | 1996

Near Infrared Spectroscopy of Highly Reddened Stars in the Galactic Plane

Masatoshi Imanishi; Yoshinori Sasaki; Miwa Goto; Naoto Kobayashi; Tetsuya Nagata; Terry Jay Jones

17--20 mag in the region within


Publications of the Astronomical Society of Japan | 2000

Subaru First-Light Deep Photometry of Galaxies in A 851 Field

Masanori Iye; Fumihide Iwamuro; Toshinori Maihara; Satoshi Miyazaki; Sadanori Okamura; Kazuhiro Shimasaku; Chris Simpson; Masayuki Akiyama; Hiroyasu Ando; T. Aoki; Tsutomu Aoki; Yoshihiro Chikada; Mamoru Doi; Noboru Ebizuka; Takeo Fukuda; Hisanori Furusawa; Miwa Goto; Masaru Hamabe; Ryuji Hata; Masahiko Hayashi; Saeko S. Hayashi; Toshihiro Horaguchi; Shin-ichi Ichikawa; Takashi Ichikawa; Masatoshi Imanishi; Katsumi Imi; Motoko Inata; Shuzo Isobe; Yoichi Itoh; Jun'ichi Iwai

sim

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