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Optimization and sensitivity of the Keck Array
S. Kernasovskiy, P. A. R. Ade, R. W. Aikin +41
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…
Optical Characterization of the Keck Array Polarimeter at the South Pole
A. G. Vieregg, P. A. R. Ade, R. Aikin +37
The Keck Array (SPUD) is a set of microwave polarimeters that observes from the South Pole at degree angular scales in search of a signature of Inflation imprinted as B-mode polari…
The source counts of submillimetre galaxies detected at 1.1 mm
K. S. Scott, G. W. Wilson, I. Aretxaga +21
The source counts of galaxies discovered at sub-millimetre and millimetre wavelengths provide important information on the evolution of infrared-bright galaxies. We combine the dat…