Zobrazeno 1 - 10
of 7 563
pro vyhledávání: '"Koyama Y"'
Publikováno v:
Journal of Pain Research, Vol Volume 12, Pp 1025-1032 (2019)
Takahiko Yoshimoto,1,2 Hiroyuki Oka,2 Tomoko Fujii,2 Kayo Kawamata,2 Akatsuki Kokaze,1 Yoshiko Koyama,3,4 Ko Matsudaira21Department of Hygiene, Public Health and Preventive Medicine, Showa University School of Medicine, Tokyo, Japan; 2Department of M
Externí odkaz:
https://doaj.org/article/4a8c290ad1f34ead94a5ea47ab9da3a8
Autor:
Kurokawa Y, Sone H, Win-Shwe TT, Zeng Y, Kimura H, Koyama Y, Yagi Y, Matsui Y, Yamazaki M, Hirano S
Publikováno v:
International Journal of Nanomedicine, Vol Volume 12, Pp 3967-3975 (2017)
Yoshika Kurokawa,1 Hideko Sone,1 Tin-Tin Win-Shwe,1 Yang Zeng,1 Hiroyuki Kimura,2 Yosuke Koyama,1 Yusuke Yagi,2 Yasuto Matsui,3 Masashi Yamazaki,4 Seishiro Hirano1 1Center for Health and Environmental Risk Research, National Institute for Environment
Externí odkaz:
https://doaj.org/article/229e503388cd404fb7a39e0e4e4e0ccc
Spectroscopic observations of PHz G237.01+42.50: A galaxy protocluster at z=2.16 in the Cosmos field
Autor:
Polletta, M., Soucail, G., Dole, H., Lehnert, M. D., Pointecouteau, E., Vietri, G., Scodeggio, M., Montier, L., Koyama, Y., Lagache, G., Frye, B. L., Cusano, F., Fumana, M.
Publikováno v:
A&A 654, A121 (2021)
The Planck satellite has identified more than 2000 protocluster candidates with extreme star formation rates (SFRs). Here, we present the spectroscopic identification of a Planck-selected protocluster located in the Cosmos field, PHz G237.01+42.50 (G
Externí odkaz:
http://arxiv.org/abs/2109.04396
Autor:
Jin, S., Dannerbauer, H., Emonts, B., Serra, P., Lagos, C. D. P., Thomson, A. P., Bassini, L., Lehnert, M., Allison, J. R., Champagne, J. B., Indermuhle, B., Norris, R. P., Seymour, N., Shimakawa, R., Casey, C. M., De Breuck, C., Drouart, G., Hatch, N., Kodama, T., Koyama, Y., Macgregor, P., Miley, G., Overzier, R., Perez-Martinez, J. M., Rodriguez-Espinosa, J. M., Rottgering, H., Portal, M. Sanchez, Ziegler, B.
Publikováno v:
A&A 652, A11 (2021)
We report a detailed CO(1-0) survey of a galaxy protocluster field at $z=2.16$, based on 475 hours of observations with the Australia Telescope Compact Array. We constructed a large mosaic of 13 individual pointings, covering an area of 21 arcmin$^2$
Externí odkaz:
http://arxiv.org/abs/2103.08884
Autor:
Cooke, E. A., Smail, Ian, Stach, S. M., Swinbank, A. M., Bower, R. G., Chen, Chian-Chou, Koyama, Y., Thomson, A. P.
We analyse 850um continuum observations of eight massive X-ray detected galaxy clusters at z~0.8-1.6 taken with SCUBA-2 on the James Clerk Maxwell Telescope. We find an average overdensity of 850um-selected sources of a factor of 4+/-2 per cluster wi
Externí odkaz:
http://arxiv.org/abs/1904.01582
Autor:
Boehm, A., Ziegler, B. L., Perez-Martinez, J. M., Kodama, T., Hayashi, M., Maier, C., Verdugo, M., Koyama, Y.
Publikováno v:
A&A 633, A131 (2020)
We observed star-forming galaxies at z~1.5 selected from the HyperSuprimeCam Subaru Strategic Program. The galaxies are part of two significant overdensities of [OII] emitters identified via narrow-band imaging and photometric redshifts from grizy ph
Externí odkaz:
http://arxiv.org/abs/1903.10016
Autor:
Aihara, H., Arimoto, N., Armstrong, R., Arnouts, S., Bahcall, N. A., Bickerton, S., Bosch, J., Bundy, K., Capak, P. L., Chan, J. H. H., Chiba, M., Coupon, J., Egami, E., Enoki, M., Finet, F., Fujimori, H., Fujimoto, S., Furusawa, H., Furusawa, J., Goto, T., Goulding, A., Greco, J. P., Greene, J. E., Gunn, J. E., Hamana, T., Harikane, Y., Hashimoto, Y., Hattori, T., Hayashi, M., Hayashi, Y., Hełminiak, K. G., Higuchi, R., Hikage, C., Ho, P. T. P., Hsieh, B. -C., Huang, K., Huang, S., Ikeda, H., Imanishi, M., Inoue, A. K., Iwasawa, K., Iwata, I., Jaelani, A. T., Jian, H. -Y., Kamata, Y., Karoji, H., Kashikawa, N., Katayama, N., Kawanomoto, S., Kayo, I., Koda, J., Koike, M., Kojima, T., Komiyama, Y., Konno, A., Koshida, S., Koyama, Y., Kusakabe, H., Leauthaud, A., Lee, C. -H., Lin, L., Lin, Y. -T., Lupton, R. H., Mandelbaum, R., Matsuoka, Y., Medezinski, E., Mineo, S., Miyama, S., Miyatake, H., Miyazaki, S., Momose, R., More, A., More, S., Moritani, Y., Moriya, T. J., Morokuma, T., Mukae, S., Murata, R., Murayama, H., Nagao, T., Nakata, F., Niida, M., Niikura, H., Nishizawa, A. J., Obuchi, Y., Oguri, M., Oishi, Y., Okabe, N., Okura, Y., Ono, Y., Onodera, M., Onoue, M., Osato, K., Ouchi, M., Price, P. A., Pyo, T. -S., Sako, M., Okamoto, S., Sawicki, M., Shibuya, T., Shimasaku, K., Shimono, A., Shirasaki, M., Silverman, J. D., Simet, M., Speagle, J., Spergel, D. N., Strauss, M. A., Sugahara, Y., Sugiyama, N., Suto, Y., Suyu, S. H., Suzuki, N., Tait, P. J., Takata, T., Takada, M., Tamura, N., Tanaka, M. M., Tanaka, M., Tanaka, Y., Terai, T., Terashima, Y., Toba, Y., Toshikawa, J., Turner, E. L., Uchida, T., Uchiyama, H., Umetsu, K., Uraguchi, F., Urata, Y., Usuda, T., Utsumi, Y., Wang, S. -Y., Wang, W. -H., Wong, K. C., Yabe, K., Yamada, Y., Yamanoi, H., Yasuda, N., Yeh, S., Yonehara, A., Yuma, S.
Publikováno v:
Publications of the Astronomical Society of Japan, Volume 70, Issue SP1, S4 (2018)
Hyper Suprime-Cam (HSC) is a wide-field imaging camera on the prime focus of the 8.2m Subaru telescope on the summit of Maunakea in Hawaii. A team of scientists from Japan, Taiwan and Princeton University is using HSC to carry out a 300-night multi-b
Externí odkaz:
http://arxiv.org/abs/1704.05858
Autor:
Dannerbauer, H., Lehnert, M. D., Emonts, B. H. C., Ziegler, B., Altieri, B., De Breuck, C., Hatch, N., Kodama, T., Koyama, Y., Kurk, J. D., Matiz, T., Miley, G., Narayanan, D., Norris, R., Overzier, R., Roettgering, H. J. A., Sargent, M., Seymour, N., Tanaka, M., Valtchanov, I., Wylezalek, D.
Publikováno v:
A&A 608, A48 (2017)
It is not yet known if the properties of molecular gas in distant protocluster galaxies are significantly affected by their environment as galaxies are in local clusters. Through a deep, 64 hours of effective on-source integration with the Australian
Externí odkaz:
http://arxiv.org/abs/1701.05250
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Autor:
Suzuki, T. L., Kodama, T., Sobral, D., Khostovan, A. A., Hayashi, M., Shimakawa, R., Koyama, Y., Tadaki, K. -i., Tanaka, I., Minowa, Y., Yamamoto, M., Smail, I., Best, P. N.
We investigate the properties of $z$=2.23 H$\alpha$ and [OIII]$\lambda$5007 emitters using the narrow-band-selected samples obtained from the High-$z$ Emission Line Survey (HiZELS: Sobral et al. 2013). We construct two samples of the H$\alpha$ and [O
Externí odkaz:
http://arxiv.org/abs/1607.02054