Now showing items 1-2 of 2

    • The QUaD Galactic Plane Survey 1: Maps And Analysis of Diffuse Emission 

      Culverhouse, T.; Ade, P.; Bock, J.; Bowden, M.; Brown, M.; Cahill, G.; Castro, P.; Church, S.; Friedman, R.; Ganga, K.; Gear, W.; Gupta, S.; Hinderks, J.; Kovac, John M; Lange, A.; Leitch, E.; Melhuish, S.; Memari, Y.; Murphy, J.; Orlando, A.; Schwarz, R.; O'Sullivan, C.; Piccirillo, L.; Pryke, C; Rajguru, N.; Rusholme, B.; Taylor, A.; Thompson, K.; Turner, A.; Wu, E.; Zemcov, M. (IOP Publishing, 2010)
      We present a survey of ∼ 800 square degrees of the galactic plane observed with the QUaD telescope. The primary product of the survey are maps of Stokes I, Q and U parameters at 100 and 150 GHz, with spatial resolution 5 ...
    • The Robinson Gravitational Wave Background Telescope (BICEP): a bolometric large angular scale CMB polarimeter 

      Yoon, K. W.; Ade, P. A. R.; Barkats, D.; Battle, J. O.; Bierman, E. M.; Bock, J. J.; Brevik, J. A.; Chiang, H. C.; Crites, A.; Dowell, C. D.; Duband, L.; Griffin, G. S.; Hivon, E. F.; Holzapfel, W. L.; Hristov, V. V.; Keating, B. G.; Kovac, John; Kuo, C. L.; Lange, A. E.; Leitch, E. M.; Mason, P. V.; Nguyen, H. T.; Ponthieu, N.; Takahashi, Y. D.; Renbarger, T.; Weintraub, L. C.; Woolsey, D. (2006)
      The Robinson Telescope (BICEP) is a ground-based millimeter-wave bolometric array designed to study the polarization of the cosmic microwave background radiation (CMB) and galactic foreground emission. Such measurements ...