Hinderks, JR;Ade, P;Bock, J;Bowden, M;Brown, ML;Cahill, G;Carlstrom, JE;Castro, PG;Church, S;Culverhouse, T;Friedman, R;Ganga, K;Gear, WK;Gupta, S;Harris, J;Haynes, V;Keating, G;Kovac, J;Kirby, E;Lange, AE;Leitch, E;Mallie, OE;Melhuish, S;Memari, Y;Murphy, A;Orlando, A;Schwarz, R;Sullivan, CO;Piccirillo, L;Pryke, C;Rajguru, N;Rusholme, B;Taylor, AN;Thompson, KL;Tucker, C;Turner, AH;Wu, EYS;Zemcov, M

2009

February

Astrophysical Journal

QUaD: A HIGH-RESOLUTION COSMIC MICROWAVE BACKGROUND POLARIMETER

Published

46 ()

ANGULAR SCALE INTERFEROMETER POLARIZATION POWER SPECTRA PROBE WMAP OBSERVATIONS OPTICAL DESIGN 2003 FLIGHT SOUTH-POLE RECEIVER BRIGHTNESS ANISOTROPY BOLOMETER

692

1221

1246

We describe the QUaD experiment, a millimeter-wavelength polarimeter designed to observe the cosmic microwave background (CMB) from a site at the South Pole. The experiment comprises a 2.64 m Cassegrain telescope equipped with a cryogenically cooled receiver containing an array of 62 polarization-sensitive bolometers. The focal plane contains pixels at two different frequency bands, 100 GHz and 150 GHz, with angular resolutions of 5' and 3'.5, respectively. The high angular resolution allows observation of CMB temperature and polarization anisotropies over a wide range of scales. The instrument commenced operation in early 2005 and collected science data during three successive Austral winter seasons of observation.

BRISTOL

0004-637X

10.1088/0004-637X/692/2/1221