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 ...
