Browsing by Author "Nagai, Makoto"

Now showing items 1-3 of 3

    • Atomic carbon in the southern Milky Way 
      Oka, Tomoharu; Kamegai, Kazuhisa; Hayashida, Masaaki; Nagai, Makoto; Ikeda, Masafumi; Kuboi, Nobuyuki; Tanaka, Kunihiko; Bronfman Aguiló, Leonardo; Yamamoto, Satoshi (UNIV CHICAGO PRESS, 2005-04-20)
      We present a coarsely sampled longitude-velocity (l-V) map of the region l = 300 degrees - 354 degrees, b = 0 degrees in the 492 GHz fine-structure transition of neutral atomic carbon (C-0 P-3(1) - P-3(0); [C I]), observed ...
    • Development of a Transportable Telescope for Galactic Survey at 500 GHz in Antarctica 
      Ishii, Shun; Masumichi, Seta; Nakai, Naomasa; Miyamoto, Yusuke; Nagai, Makoto; Arai, Hitoshi; Maezawa, Hiroyuki; Taketo, Nagasaki; Miyagawa, Naoki; Motoyama, Hideaki; Sekimoto, Yutaro; Bronfman Aguiló, Leonardo (2013-01)
      We have developed a transportable 30-cm submillimeter- wave telescope to operate at the Dome Fuji station in the Antarctic plateau. Transportability is an important requirement in the design; the telescope can be divided ...
    • SECOND SEASON QUIET OBSERVATIONS: MEASUREMENTS OF THE COSMIC MICROWAVE BACKGROUND POLARIZATION POWER SPECTRUM ... 
      Araujo, D.; Bischoff, C.; Brizius, A; Buder, I.; Chinone, Y.; Cleary, K.; Dumoulin, R. N.; Kusaka, A.; Monsalve, R.; Næss, S. K.; Newburgh, L. B.; Reeves, R.; Wehus, I. K.; Zwart, J. T. L.; Bronfman Aguiló, Leonardo; Bustos, R.; Church, S. E.; Dickinson, C.; Eriksen, H. K.; Gaier, T.; Gundersen, J. O.; Hasegawa, M.; Hazumi, M.; Huffenberger, K. M.; Ishidoshiro, K.; Jones, M. E.; Kangaslahti, P.; Kapner, D. J.; Kubik, D.; Lawrence, C. R.; Limon, M.; McMahon, J. J.; Miller, A. D.; Nagai, Makoto; Nguyen, H.; Nixon, G.; Pearson, T. J.; Piccirillo, L.; Radford, S. J. E.; Readhead, A. C. S.; Richards, J. L.; Samtleben, D.; Seiffert, M.; Shepherd, M. C.; Smith, K.; Staggs, S. T.; Tajima, O.; Thompson, K. L.; Vanderlinde, K.; Williamson, R. (IOP PUBLISHING LTD, 2012-12)
      The Q/U Imaging ExperimenT (QUIET) has observed the cosmic microwave background (CMB) at 43 and 95 GHz. The 43 GHz results have been published in a previous paper, and here we report the measurement of CMB polarization ...