Zobrazeno 1 - 10
of 31
pro vyhledávání: '"Savage, R. S."'
Autor:
Todorović, M., Davies, R. D., Dickinson, C., Davis, R. J., Cleary, K. A., Genova-Santos, R., Grainge, K. J. B., Hafez, Y. A., Hobson, M. P., Jones, M. E., Lancaster, K., Rebolo, R., Reich, W., Rubiño-Martin, J. A., Saunders, R. D. E., Savage, R. S., Scott, P. F., Slosar, A., Taylor, A. C., Watson, R. A.
The Very Small Array (VSA) has been used to survey the l = 27 to 46 deg, |b|<4 deg region of the Galactic plane at a resolution of 13 arcmin. The survey consists of 44 pointings of the VSA, each with a r.m.s. sensitivity of ~90 mJy/beam. These data a
Externí odkaz:
http://arxiv.org/abs/1006.2770
Autor:
Clements, D. L., Vaccari, M., Babbedge, T., Oliver, S., Rowan-Robinson, M., Davoodi, P., Ivison, R., Farrah, D., Dunlop, J., Shupe, Dave, Waddington, I., Simpson, C., Furusawa, H., Serjeant, S., Afonso-Luis, A., Alexander, D. M., Aretxaga, I., Blain, A., Borys, C., Chapman, S., Coppin, K., Dunne, L., Dye, S., Eales, S. A., Evans, T., Fang, F., Frayer, D., Fox, M., Gear, W. K., Greve, T. R., Halpern, M., Hughes, D. H., Jenness, T., Lonsdale, C. J., Mortier, A. M. J., Page, M. J., Pope, A., Priddey, R. S., Rawlings, S., Savage, R. S., Scott, D., Scott, S. E., Sekiguchi, K., Smail, I., Smith, H. E., Stevens, J. A., Surace, J., Takagi, T., van Kampen, E.
We present the optical-to-submm spectral energy distributions for 33 radio & mid-IR identified submillimetre galaxies discovered via the SHADES 850 micron SCUBA imaging in the Subaru-XMM Deep Field (SXDF). Optical data for the sources comes from the
Externí odkaz:
http://arxiv.org/abs/0803.0475
Autor:
Berta, S., Lonsdale, C. J., Polletta, M., Savage, R. S., Franceschini, A., Buttery, H., Cimatti, A., Dias, J., Feruglio, C., Fiore, F., Held, E. V., La Franca, F., Maiolino, R., Marconi, A., Matute, I., Oliver, S. J., Ricciardelli, E., Rubele, S., Sacchi, N., Shupe, D., Surace, J.
Publikováno v:
Astron.Astrophys.476:1,2007
(Abridged) We selected high-z massive galaxies at 5.8 microns, in the SWIRE ELAIS-S1 field (1 sq. deg.). Galaxies with the 1.6 microns stellar peak redshifted into the IRAC bands (z~1-3, called ``IR-peakers'') were identified. Stellar masses were der
Externí odkaz:
http://arxiv.org/abs/0710.0300
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:
Takagi, T., Matsuhara, H., Wada, T., Oyabu, S., Imai, K., Pearson, C. P., Hanami, H., Onaka, T., Fujishiro, N., Ishihara, D., Ita, Y., Kataza, H., Kim, W., Matsumoto, T., Murakami, H., Ohyama, Y., Sakon, I., Tanabe, T., Uemizu, K., Ueno, M., Watarai, H., Usui, F., Lee, H. M., Im, M., Serjeant, S., Savage, R. S., Tange, T., Nakagawa, T.
We present an initial analysis of AKARI 18um-selected galaxies using all 9 photometric bands at 2-24um available in the InfraRed Camera (IRC), in order to demonstrate new capabilities of AKARI cosmological surveys. We detected 72 sources at 18um in a
Externí odkaz:
http://arxiv.org/abs/0705.1365
Autor:
Ivison, R. J., Greve, T. R., Dunlop, J. S., Peacock, J. A., Egami, E., Smail, Ian, Ibar, E., van Kampen, E., Aretxaga, I., Babbedge, T., Biggs, A. D., Blain, A. W., Chapman, S. C., Clements, D. L., Coppin, K., Farrah, D., Halpern, M., Hughes, D. H., Jarvis, M. J., Jenness, T., Jones, J. R., Mortier, A. M. J., Oliver, S., Papovich, C., Perez-Gonzalez, P. G., Pope, A., Rawlings, S., Rieke, G. H., Rowan-Robinson, M., Savage, R. S., Scott, D., Seigar, M., Serjeant, S., Simpson, C., Stevens, J. A., Vaccari, M., Wagg, J., Willott, C. J.
Publikováno v:
Mon.Not.Roy.Astron.Soc.380:199-228,2007
Determining an accurate position for a submm galaxy (SMG) is the crucial step that enables us to move from the basic properties of an SMG sample - source counts and 2-D clustering - to an assessment of their detailed, multi-wavelength properties, the
Externí odkaz:
http://arxiv.org/abs/astro-ph/0702544
Autor:
Coppin, K., Chapin, E. L., Mortier, A. M. J., Scott, S. E., Borys, C., Dunlop, J. S., Halpern, M., Hughes, D. H., Pope, A., Scott, D., Serjeant, S., Wagg, J., Alexander, D. M., Almaini, O., Aretxaga, I., Babbedge, T., Best, P. N., Blain, A., Chapman, S., Clements, D. L., Crawford, M., Dunne, L., Eales, S. A., Edge, A. C., Farrah, D., Gaztanaga, E., Gear, W. K., Granato, G. L., Greve, T. R., Fox, M., Ivison, R. J., Jarvis, M. J., Jenness, T., Lacey, C., Lepage, K., Mann, R. G., Marsden, G., Martinez-Sansigre, A., Oliver, S., Page, M. J., Peacock, J. A., Pearson, C. P., Percival, W. J., Priddey, R. S., Rawlings, S., Rowan-Robinson, M., Savage, R. S., Seigar, M., Sekiguchi, K., Silva, L., Simpson, C., Smail, I., Stevens, J. A., Takagi, T., Vaccari, M., van Kampen, E., Willott, C. J.
Publikováno v:
Mon.Not.Roy.Astron.Soc.372:1621-1652,2006
We present the maps, source catalogue and number counts of the largest, most complete and unbiased extragalactic submillimetre survey ever undertaken: the 850-micron SCUBA HAlf Degree Extragalactic Survey (SHADES). Using the Submillimetre Common-User
Externí odkaz:
http://arxiv.org/abs/astro-ph/0609039
Autor:
Rajguru, N., Myers, S. T., Battye, R. A., Bond, J. Richard, Cleary, K., Contaldi, C. R., Davies, R. D., Davis, R. J., Dickinson, C., Genova-Santos, R., Grainge, K., Hafez, Y. A., Hobson, M. P., Jones, M. E., Kneissl, R., Lancaster, K., Lasenby, A., Mason, B. S., Pearson, T. J., Pooley, G. G., Readhead, A. C. S., Rebolo, R., Rocha, G., Rubino-Martin, J. A., Saunders, R. D. E., Savage, R. S., Scaife, A., Scott, P. F., Sievers, J. L., Slosar, A., Taylor, A. C., Titterington, D., Waldram, E., Watson, R. A., Wilkinson, A.
Publikováno v:
Mon.Not.Roy.Astron.Soc. 363 (2005) 1125-1135
We present coincident observations of the Cosmic Microwave Background (CMB) from the Very Small Array (VSA) and Cosmic Background Imager (CBI) telescopes. The consistency of the full datasets is tested in the map plane and the Fourier plane, prior to
Externí odkaz:
http://arxiv.org/abs/astro-ph/0502330
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Akademický článek
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