Now showing items 1-4 of 4

    • BICEP3 focal plane design and detector performance 

      Hui, H.; Ade, P. A. R.; Ahmed, Z.; Alexander, Kate Denham; Amiri, M.; Barkats, Denis A.; Benton, S. J.; Bischoff, Colin A.; Bock, J. J.; Boenish, H.; Bowens-Rubin, R; Buder, I; Bullock, E.; Buza, Victor; Connors, Jake Anthony; Filippini, J. P.; Fliescher, S.; Grayson, J. A.; Halpern, M.; Harrison, Sarah; Hilton, G. C.; Hristov, V. V.; Irwin, K. D.; Kang, J.; Karkare, Kirit Sukrit; Karpel, E.; Kefeli, S.; Kernasovskiy, S. A.; Kovac, John M; Kuo, C. L.; Leitch, E. M.; Lueker, M.; Megerian, K. G.; Monticue, V.; Namikawa, T.; Netterfield, C. B.; Nguyen, H. T.; O, R.; Ogburn, R. W.; Pryke, C; Reintsema, C. D.; Richter, Sonja Valeska; Schwarz, R.; Sorensen, C.; Sheehy, C. D.; Staniszewski, Z. K.; Steinbach, B.; Teply, G. P.; Thompson, K. L.; Tolan, J. E.; Tucker, C.; Turner, A. D.; Vieregg, A. G.; Wandui, A.; Weber, A. C.; Wiebe, D. V.; Willmert, J.; Wu, W. L. K.; Yoon, K. W. (SPIE, 2016)
      BICEP3, the latest telescope in the BICEP/Keck program, started science observations in March 2016. It is a 550mm aperture refractive telescope observing the polarization of the cosmic microwave background at 95 GHz. We ...
    • BICEP3 performance overview and planned Keck Array upgrade 

      Grayson, J. A.; Ade, P. A. R.; Ahmed, Z.; Alexander, Kate Denham; Amiri, M.; Barkats, Denis A.; Benton, S. J.; Bischoff, Colin A.; Bock, J. J.; Boenish, H.; Bowens-Rubin, R; Buder, I; Bullock, E.; Buza, Victor; Connors, Jake Anthony; Filippini, J. P.; Fliescher, S.; Halpern, M.; Harrison, Sarah; Hilton, G. C.; Hristov, V. V.; Hui, H.; Irwin, K. D.; Kang, J.; Karkare, Kirit Sukrit; Karpel, E.; Kefeli, S.; Kernasovskiy, S. A.; Kovac, John M; Kuo, C. L.; Leitch, E. M.; Lueker, M.; Megerian, K. G.; Monticue, V.; Namikawa, T.; Netterfield, C. B.; Nguyen, H. T.; O, R.; Ogburn, R. W.; Pryke, C; Reintsema, C. D.; Richter, Sonja Valeska; Schwarz, R.; Sorenson, C.; Sheehy, C. D.; Staniszewski, Z. K.; Steinbach, B.; Teply, G. P.; Thompson, K. L.; Tolan, J. E.; Tucker, C.; Turner, A. D.; Vieregg, A. G.; Wandui, A.; Weber, A. C.; Wiebe, D. V.; Willmert, J.; Wu, W. L. K.; Yoon, K. W. (2016)
      Bicep3 is a 520 mm aperture, compact two-lens refractor designed to observe the polarization of the cosmic microwave background (CMB) at 95 GHz. Its focal plane consists of modularized tiles of antenna-coupled transition ...
    • BICEP3: A 95GHz Refracting Telescope for Degree-Scale CMB Polarization 

      Ahmed, Z.; Amiri, M.; Benton, S. J.; Bock, J. J.; Bowens-Rubin, R; Buder, I; Bullock, E.; Connors, Jake Anthony; Filippini, J. P.; Grayson, J. A.; Halpern, M.; Hilton, G. C.; Hristov, V. V.; Hui, H.; Irwin, K. D.; Kang, J.; Karkare, Kirit Sukrit; Karpel, E.; Kovac, John M; Kuo, C. L.; Netterfield, C. B.; Nguyen, H. T.; O, R.; Ogburn, R. W.; Pryke, C; Reintsema, C. D.; Richter, Sonja Valeska; Thompson, K. L.; Turner, A. D.; Vieregg, A. G.; Wu, W. L. K.; Yoon, K. W. (International Society for Optics and Photonics, 2014)
      Bicep3 is a 550 mm-aperture refracting telescope for polarimetry of radiation in the cosmic microwave background at 95 GHz. It adopts the methodology of Bicep1, Bicep2 and the Keck Array experiments — it possesses sufficient ...
    • Optimization and sensitivity of the Keck array 

      Kernasovskiy, S.; Ade, P. A. R.; Aikin, R. W.; Amiri, M.; Benton, S.; Bischoff, Colin A.; Bock, J. J.; Bonetti, J. A.; Brevik, J. A.; Burger, B.; Davis, G.; Dowell, C. D.; Duband, L.; Filippini, J. P.; Fliescher, S.; Golwala, S. R.; Halpern, M.; Hasselfield, M.; Hilton, G.; Hristov, V. V.; Irwin, K.; Kovac, John M; Kuo, C. L.; Leitch, E.; Lueker, M.; Netterfield, C. B.; Nguyen, H. T.; O, R.; Ogburn, R. W.; Pryke, C; Reintsema, C.; Ruhl, J. E.; Runyan, M. C.; Schwarz, R.; Sheehy, C. D.; Staniszewski, Z.; Sudiwala, R.; Teply, G.; Tolan, J. E.; Turner, A. D.; Vieregg, A.; Wiebe, D. V.; Wilson, P.; Wong, C. L. (International Society for Optics and Photonics, 2012)
      The Keck Array (SPUD) began observing the cosmic microwave background’s polarization in the winter of 2011 at the South Pole. The Keck Array follows the success of the predecessor experiments Bicep and Bicep2,1 using five ...