Zobrazeno 1 - 10
of 182
pro vyhledávání: '"Ootsubo, T."'
Autor:
Arimatsu, K., Tsumura, K., Usui, F., Shinnaka, Y., Ichikawa, K., Ootsubo, T., Kotani, T., Wada, T., Nagase, K., Watanabe, J.
Publikováno v:
Nature Astronomy, 3, pages 301-306 (2019)
Kuiper belt objects (KBOs) are thought to be the remnant of the early solar system, and their size distribution provides an opportunity to explore the formation and evolution of the outer solar system. In particular, the size distribution of kilometr
Externí odkaz:
http://arxiv.org/abs/1910.09994
Autor:
Ishihara, D., Kondo, T., Kaneda, H., Suzuki, T., Nakamichi, K., Takaba, S., Kobayashi, H., Masuda, S., Ootsubo, T., Pyo, J., Onaka, T.
Context. We are creating the AKARI mid-infrared all-sky diffuse maps. Through a foreground removal of the zodiacal emission, we serendipitously detected a bright residual component whose angular size is about 50 x 20 deg. at a wavelength of 9 micron.
Externí odkaz:
http://arxiv.org/abs/1705.01541
Autor:
Kondo, T., Ishihara, D., Kaneda, H., Nakamichi, K., Takaba, S., Kobayashi, H., Ootsubo, T., Pyo, J., Onaka, T.
The zodiacal emission, which is the thermal infrared (IR) emission from the interplanetary dust (IPD) in our Solar System, has been studied for a long time. Nevertheless, accurate modeling of the zodiacal emission has not been successful to reproduce
Externí odkaz:
http://arxiv.org/abs/1601.05553
Autor:
Mueller, T. G., Miyata, T., Kiss, C., Gurwell, M. A., Hasegawa, S., Vilenius, E., Sako, S., Kamizuka, T., Nakamura, T., Asano, K., Uchiyama, M., Konishi, M., Yoneda, M., Ootsubo, T., Usui, F., Yoshii, Y., Kidger, M., Altieri, B., Lorente, R., Pal, A., O'Rourke, L., Metcalfe, L.
The near-Earth asteroid (308635) 2005 YU55 is a potentially hazardous asteroid which was discovered in 2005 and passed Earth on November 8th 2011 at 0.85 lunar distances. This was the closest known approach by an asteroid of several hundred metre dia
Externí odkaz:
http://arxiv.org/abs/1307.7517
Autor:
Murakami, H., Baba, H., Barthel, P., Clements, D. L., Cohen, M., Doi, Y., Enya, K., Figueredo, E., Fujishiro, N., Fujiwara, H., Fujiwara, M., Garcia-Lario, P., Goto, T., Hasegawa, S., Hibi, Y., Hirao, T., Hiromoto, N., Hong, S. S., Imai, K., Ishigaki, M., Ishiguro, M., Ishihara, D., Ita, Y., Jeong, W. -S., Jeong, K. S., Kaneda, H., Kataza, H., Kawada, M., Kawai, T., Kawamura, A., Kessler, M. F., Kester, Do, Kii, T., Kim, D. C., Kim, W., Kobayashi, H., Koo, B. C., Kwon, S. M., Lee, H. M., Lorente, R., Makiuti, S., Matsuhara, H., Matsumoto, T., Matsuo, H., Matsuura, S., Mueller, T. G., Murakami, N., Nagata, H., Nakagawa, T., Naoi, T., Narita, M., Noda, M., Oh, S. H., Ohnishi, A., Ohyama, Y., Okada, Y., Okuda, H., Oliver, S., Onaka, T., Ootsubo, T., Oyabu, S., Pak, S., Park, Y. S., Pearson, C. P., Rowan-Robinson, M., Saito, T., Sakon, I., Salama, A., Sato, S., Savage, R. S., Serjeant, S., Shibai, H., Shirahata, M., Sohn, J. J., Suzuki, T., Takagi, T., Takahashi, H., Tanabe, T., Takeuchi, T. T., Takita, S., Thomson, M., Uemizu, K., Ueno, M., Usui, F., Verdugo, E., Wada, T., Wang, L., Watabe, T., Watarai, H., White, G. J., Yamamura, I., Yamauchi, C., Yasuda, A.
Publikováno v:
Publ.Astron.Soc.Jap.59:369-376,2007
AKARI, the first Japanese satellite dedicated to infrared astronomy, was launched on 2006 February 21, and started observations in May of the same year. AKARI has a 68.5 cm cooled telescope, together with two focal-plane instruments, which survey the
Externí odkaz:
http://arxiv.org/abs/0708.1796
Autor:
Onaka, T., Matsuhara, H., Wada, T., Fujishiro, N., Fujiwara, H., Ishigaki, M., Ishihara, D., Ita, Y., Kataza, H., Kim, W., Matsumoto, T., Murakami, H., Ohyama, Y., Oyabu, S., Sakon, I., Tanabe, T., Takagi, T., Uemizu, K., Ueno, M., Usui, F., Watarai, H., Cohen, M., Enya, K., Ootsubo, T., Pearson, C. P., Takeyama, N., Yamamuro, T., Ikeda, Y.
The Infrared Camera (IRC) is one of two focal-plane instruments on the AKARI satellite. It is designed for wide-field deep imaging and low-resolution spectroscopy in the near- to mid-infrared (1.8--26.5um) in the pointed observation mode of AKARI. IR
Externí odkaz:
http://arxiv.org/abs/0705.4144
Publikováno v:
Astrophys.J.662:1282-1292,2007
The core-accretion and disk instability models have so far been used to explain planetary formation. These models have different conditions, such as planet mass, disk mass, and metallicity for formation of gas giants. The core-accretion model has a m
Externí odkaz:
http://arxiv.org/abs/astro-ph/0703237
Autor:
Matsuura, M., Yamamura, I., Murakami, H., Onaka, T., Ootsubo, T., Tohya, T., Okamura, Y., Freund, M. M., Tanaka, Masahiro
Results of an SiO maser survey for the late-type stars selected by the IRTS (Infrared Telescope in Space) are presented. We have detected SiO J=1-0, v=1 and/or v=2 lines in 27 stars out of 59 stars. The maser intensity increases with the depth of the
Externí odkaz:
http://arxiv.org/abs/astro-ph/0006009
Autor:
Meech, K. J., Ageorges, N., Arpigny, C., Ates, A., Aycock, J., Bagnulo, S., Bailey, J., Barber, R., Barrera, L., Barrena, R., Bauer, J. M., Belton, M. J. S., Bensch, F., Bhattacharya, B., Biver, N., Blake, G., Bockelée-Morvan, D., Boehnhardt, H., Bonev, B. P., Bonev, T., Buie, M. W., Burton, M. G., Butner, H. M., Cabanac, R., Campbell, R., Campins, H., Capria, M. T., Carroll, T., Chaffee, F., Charnley, S. B., Cleis, R., Coates, A., Cochran, A., Colom, P., Conrad, A., Coulson, I. M., Crovisier, J., deBuizer, J., Dekany, R., de Léon, J., Russo, N. Dello, Delsanti, A., DiSanti, M., Drummond, J., Dundon, L., Etzel, P. B., Farnham, T. L., Feldman, P., Fernández, Y. R., Filipovic, M. D., Fisher, S., Fitzsimmons, A., Fong, D., Fugate, R., Fujiwara, H., Fujiyoshi, T., Furusho, R., Fuse, T., Gibb, E., Groussin, O., Gulkis, S., Gurwell, M., Hadamcik, E., Hainaut, O., Harker, D., Harrington, D., Harwit, M., Hasegawa, S., Hergenrother, C. W., Hirst, P., Hodapp, K., Honda, M., Howell, E. S., Hutsemékers, D., Iono, D., Jackson, W., Jehin, E., Jiang, Z. J., Jones, G. H., Jones, P. A., Kadono, T., Kamath, U. W., Käufl, H. U., Kasuga, T., Kawakita, H., Kelley, M. S., Kerber, F., Kidger, M., Kinoshita, D., Knight, M., Lara, L., Larson, S. M., Lederer, S., Levasseur-Regourd, A. C., Li, J. Y., Licandro, J., Lisse, C. M., LoCurto, G., Lovell, A. J., Lowry, S. C., Lyke, J., Lynch, D., Ma, J., Magee-Sauer, K., Maheswar, G., Manfroid, J., Marco, O., Martin, P., Melnick, G., Miller, S., Miyata, T., Moriarty-Schieven, G. H., Moskovitz, N., Mueller, B. E. A., Mumma, M. J., Muneer, S., Neufeld, D. A., Ootsubo, T., Osip, D., Pandea, S. K., Pantin, E., Paterno-Mahler, R., Patten, B., Penprase, B. E., Peck, A., Petitas, G., Pinilla-Alonso, N., Pittichova, J., Pompei, E., Prabhu, T. P., Qi, C., Rao, R., Rauer, H., Reitsema, H., Rodgers, S. D., Rodriguez, P., Ruane, R., Ruch, G., Rujopakarn, W., Sahu, D. K., Sako, S., Sakon, I., Samarasinha, N., Sarkissian, J. M., Saviane, I., Schirmer, M., Schultz, P., Schulz, R., Seitzer, P., Sekiguchi, T., Selman, F., Serra-Ricart, M., Sharp, R., Snell, R. L., Snodgrass, C., Stallard, T., Stecklein, G., Sterken, C., Stüwe, J. A., Sugita, S., Sumner, M., Suntzeff, N., Swaters, R., Takakuwa, S., Takato, N., Thomas-Osip, J., Thompson, E., Tokunaga, A. T., Tozzi, G. P., Tran, H., Troy, M., Trujillo, C., Van Cleve, J., Vasundhara, R., Vazquez, R., Vilas, F., Villanueva, G., von Braun, K., Vora, P., Wainscoat, R. J., Walsh, K., Watanabe, J., Weaver, H. A., Weaver, W., Weiler, M., Weissman, P. R., Welsh, W. F., Wilner, D., Wolk, S., Womack, M., Wooden, D., Woodney, L. M., Woodward, C., Yamashita, T., Yang, B., Yokogawa, S., Zook, A. C., Zauderer, A., Zhao, X., Zhou, X.
Publikováno v:
Science, 2005 Oct . 310(5746), 265-269.
Externí odkaz:
https://www.jstor.org/stable/3842647
Autor:
Sugita, S., Ootsubo, T., Kadono, T., Honda, M., Sako, S., Miyata, T., Sakon, I., Yamashita, T., Kawakita, H., Fujlwara, H., Fujiyoshi, T., Takato, N., Fuse, T., Watanabe, J., Furusho, R., Hasegawa, S., Kasuga, T., Sekiguchi, T., Kinoshita, D., Meech, K. J., Wooden, D. H., Ip, W. H.
Publikováno v:
Science, 2005 Oct . 310(5746), 274-278.
Externí odkaz:
https://www.jstor.org/stable/3842649