Zobrazeno 1 - 10
of 1 360
pro vyhledávání: '"Oya S"'
Autor:
Davidge, T. J., Andersen, D. R., Lardiere, O., Bradley, C., Blain, C., Oya, S., Terada, H., Hayano, Y., Lamb, M., Akiyama, M., Ono, Y. H., Suzuki, G.
We discuss images of the star clusters GLIMPSE C01 (GC01) and GLIMPSE C02 (GC02) that were recorded with the Subaru IRCS. Distortions in the wavefront were corrected with the RAVEN adaptive optics (AO) science demonstrator, allowing individual stars
Externí odkaz:
http://arxiv.org/abs/1610.09484
Autor:
Zamora Navas, P., Montañez Heredia, E., Nieto Orellana, J., Gónzalez García, C., Cano Obando, L., Cárdenas Rebollo, L., Abderrachid Al Chaid, Y., Saadouli Arco, M., Rodríguez Delourme, I., Díez Izquierdo, M., Prado Martín de Lucía, L.F., Durán Garrido, J., Fernández Hijano, M., Víquez da Silva, R., Olofsson Suárez-Bárcena, C., Jiménez Garrido, C., García Vera, J.J., Pérez Cardeña, J., Irízar Jiménez, S., Esteban del Castillo, J.L., García Píriz, M., Gómez Palomo, J.M., Fernández Martín, F.J.A., Huertas Segador, P., Santos de la Fuente, J., Serrano Fernández, J., Estades Rubio, F., Fernández de Rota, A., García Herrera, J.M., Leiva Gea, A., Lombardo Torre, M., Mariscal Lara, J., Martín Castilla, B., Urbano Labajos, V., Sánchez García, A., Quirante Sánchez, V., Cañada Oya, S., Rodríguez Jiménez, M., Delgado Rufino, B., Queipo de Llano Temboury, A., Barón Romero, M., López Hermoso, M.D., Benavente Casajús, M., Loring Caffarena, T., Chaparro Villar, M.A., de la Torre Solís, F.
Publikováno v:
In Revista Espanola de Cirugia Ortopedica y Traumatologia January-February 2021 65(1):54-62
Autor:
Davidge, T. J., Andersen, D. R., Lardiere, O., Bradley, C., Blain, C., Oya, S., Akiyama, M., Ono, Y. H.
Near-infrared (NIR) spectra that have an angular resolution of ~ 0.15 arcsec are used to examine the stellar content of the central regions of the nearby elliptical galaxy Maffei 1. The spectra were recorded at the Subaru Telescope, with wavefront di
Externí odkaz:
http://arxiv.org/abs/1509.04338
Autor:
Enya, K., Kotani, T., Haze, K., Aono, K., Nakagawa, T., Matsuhara, H., Kataza, H., Wada, T., Kawada, M., Fujiwara, K., Mita, M., Takeuchi, S., Komatsu, K., Sakai, S., Uchida, H., Mitani, S., Yamawaki, T., Miyata, T., Sako, S., Nakamura, T., Asano, K., Yamashita, T., Narita, N., Matsuo, T., Tamura, M., Nishikawa, J., Kokubo, E., Hayano, Y., Oya, S., Fukagawa, M., Shibai, H., Baba, N., Murakami, N., Itoh, Y., Honda, M., Okamoto, B., Ida, S., Takami, M., Abe, L., Guyon, O., Bierden, P., Yamamuro, T.
Publikováno v:
AdSR, 48, 323 (2011)
We present the SPICA Coronagraphic Instrument (SCI), which has been designed for a concentrated study of extra-solar planets (exoplanets). SPICA mission provides us with a unique opportunity to make high contrast observations because of its large tel
Externí odkaz:
http://arxiv.org/abs/1108.3157
Autor:
Goto, M., Henning, Th., Kouchi, A., Takami, H., Hayano, Y., Usuda, T., Takato, N., Terada, H., Oya, S., Jäger, C., Andersen, A. C.
Publikováno v:
Astrophys.J.693:610-616,2009
We present spatially resolved 3 um spectra of Elias 1 obtained with an adaptive optics system. The central part of the disk is almost devoid of PAH emission at 3.3 um; it shows up only at 30 AU and beyond. The PAH emission extends up to 100 AU, at le
Externí odkaz:
http://arxiv.org/abs/0811.2220
Autor:
Goto, M., Kwok, Sun, Takami, H., Hayashi, M., Gaessler, W., Hayano, Y., Iye, M., Kamata, Y., Kanzawa, T., Kobayashi, N., Minowa, Y., Nedachi, K., Oya, S., Pyo, T. -S., Saint-Jacques, D., Takato, N., Terada, H., Henning, Th.
Publikováno v:
Astrophys.J.662:389-394,2007
We present 3 um spectroscopy of the carbon-rich proto-planetary nebulae IRAS 04296+3429 and IRAS 05341+0852 conducted with the adaptive optics system at the Subaru Telescope. We utilize the nearly diffraction-limited spectroscopy to probe the spatial
Externí odkaz:
http://arxiv.org/abs/astro-ph/0611916
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:
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:
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
Autor:
Iwamuro, F., Motohara, K., Maihara, T., Iwai, J., Tanabe, H., Taguchi, T., Hata, R., Terada, T., Goto, M., Oya, S., team, Subaru project
We present high spatial resolution images of the gravitational-lens system PG 1115+080 taken with the near-infrared camera (CISCO) on the Subaru telescope. The FWHM of the combined image is $0.''32$ in the $K'$-band, yielding spatial resolution of $0
Externí odkaz:
http://arxiv.org/abs/astro-ph/0001051