Zobrazeno 1 - 10
of 898
pro vyhledávání: '"Hata, R."'
Publikováno v:
In Public Health January 2024 226:255-260
Publikováno v:
In Public Health November 2023 224:8-13
Akademický článek
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Autor:
Motohara, K., Iwamuro, F., Maihara, T., Oya, S., Tsukamoto, H., Imanishi, M., Terada, H., Goto, M., Iwai, J., Tanabe, H., Hata, R., Taguchi, T., Harashima, T.
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
Externí odkaz:
http://arxiv.org/abs/astro-ph/0203320
Autor:
Motohara, K., Yamada, T., Iwamuro, F., Hata, R., Taguchi, T., Harashima, T., Maihara, T., Iye, M., Simpson, C., Yoshida, M.
We present low-resolution, near-IR JHK spectra of the weak z=2.39 radio galaxy 53W002, obtained with the OH-airglow Suppressor spectrograph (OHS) and Cooled Infrared Spectrograph and Camera for OHS (CISCO) on the Subaru Telescope. They cover rest-fra
Externí odkaz:
http://arxiv.org/abs/astro-ph/0104473
This paper describes an OH-airglow Suppressor (OHS) for the infrared Nasmyth focus of the Subaru telescope. OHS has the capability of eliminating 224 airglow-lines in the $J$- and $H$-bands, which are major sources of background radiation at near-inf
Externí odkaz:
http://arxiv.org/abs/astro-ph/0101076
Autor:
Maihara, T., Iwamuro, F., Tanabe, H., Taguchi, T., Hata, R., Oya, S., Kashikawa, N., Iye, M., Miyazaki, S., Karoji, H., Yoshida, M., Totani, T., Yoshii, Y., Okamura, S., Shimasaku, K., Saito, Y., Ando, H., Goto, M., Hayashi, M., Kaifu, N., Kobayashi, N., Kosugi, G., Motohara, K., Nishimura, T., Noumaru, J., Ogasawara, R., Sasaki, T., Sekiguchi, K., Takata, T., Terada, H., Yamashita, T., Usuda, T., Tokunaga, A. T.
Deep near-infrared images of a blank 2'x2' section of sky near the Galactic north pole taken by Subaru Telescope are presented. The total integration times of the J and K' bands are 12.1 hours and 9.7 hours, resulting in 5-sigma limiting magnitudes o
Externí odkaz:
http://arxiv.org/abs/astro-ph/0009409
Autor:
Nakajima, T., Iwamuro, F., Maihara, T., Motohara, K., Terada, H., Goto, M., Iwai, J., Tanabe, H., Taguchi, T., Hata, R., Yanagisawa, K., Iye, M., Kashikawa, N., Tamura, M.
We construct infrared star count models of the Galaxy applicable at faint magnitudes. In addition to dwarfs and subdwarfs, we also take into account L dwarfs, T dwarfs, and white dwarfs of both disk and halo. As a test case of the models, we analyze
Externí odkaz:
http://arxiv.org/abs/astro-ph/0008004
Autor:
Ohta, K., Matsumoto, T., Maihara, T., Iwamuro, F., Terada, H., Goto, M., Motohara, K., Taguchi, T., Hata, R., Yoshida, M., Iye, M., Simpson, C., Takata, T.
Results of a narrow-band imaging for the redshifted [OII]3727 emission around a quasar at z=4.7 obtained with the Subaru telescope and CISCO (a Cassegrain near infrared camera) are presented. A significant emission line is detected in the narrow-band
Externí odkaz:
http://arxiv.org/abs/astro-ph/0003107
Autor:
Iwamuro, F., Motohara, K., Maihara, T., Iwai, J., Tanabe, H., Taguchi, T., Hata, R., Terada, H., Goto, M., Oya, S., Iye, M., Yoshida, M., Karoji, H., Ogasawara, R., Sekiguchi, K.
We present the 2.12~$\mu$m narrow-band image of the Hubble Deep Field North taken with the near-infrared camera (CISCO) on the Subaru telescope. Among five targets whose H$\alpha$ or [O~{\sc iii}] emission lines are redshifted into our narrow-band ra
Externí odkaz:
http://arxiv.org/abs/astro-ph/0001050