QUaD: A high-resolution cosmic microwave background polarimeter

J. R. Hinderks; P. Ade; J. Bock; M. Bowden; M. L. Brown; G. Cahill; J. E. Carlstrom; P. G. Castro; S. Church; T. Culverhouse; R. Friedman; K. Ganga; W. K. Gear; S. Gupta; J. Harris; V. Haynes; B. G. Keating; J. Kovac; E. Kirby; A. E. Lange; E. Leitch; O. E. Mallie; S. Melhuish; Y. Memari; A. Murphy; A. Orlando; R. Schwarz; C. O'Sullivan; L. Piccirillo; C. Pryke; N. Rajguru; B. Rusholme; A. N. Taylor; K. L. Thompson; C. Tucker; A. H. Turner; E. Y.S. Wu; M. Zemcov

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

QUaD: A high-resolution cosmic microwave background polarimeter

J. R. Hinderks
, P. Ade
, J. Bock
, M. Bowden
, M. L. Brown
, G. Cahill
, J. E. Carlstrom
, P. G. Castro
, S. Church
, T. Culverhouse
, R. Friedman
, K. Ganga
, W. K. Gear
, S. Gupta
, J. Harris
, V. Haynes
, B. G. Keating
, J. Kovac
, E. Kirby
, A. E. Lange

E. Leitch, O. E. Mallie, S. Melhuish, Y. Memari, A. Murphy, A. Orlando, R. Schwarz, C. O'Sullivan, L. Piccirillo, C. Pryke, N. Rajguru, B. Rusholme, A. N. Taylor, K. L. Thompson, C. Tucker, A. H. Turner, E. Y.S. Wu, M. Zemcov

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Abstract

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 35, 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.

Original language	English
Pages (from-to)	1221-1246
Number of pages	26
Journal	Astrophysical Journal
Volume	692
Issue number	2
DOIs	https://doi.org/10.1088/0004-637X/692/2/1221
Publication status	Published - 20 Feb 2009

Keywords

cosmic microwave background
instrumentation: polarimeters

Authors (Note for portal: view the doc link for the full list of authors)

Authors
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

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

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Hinderks, J. R., Ade, P., Bock, J., Bowden, M., Brown, M. L., Cahill, G., Carlstrom, J. E., Castro, P. G., Church, S., Culverhouse, T., Friedman, R., Ganga, K., Gear, W. K., Gupta, S., Harris, J., Haynes, V., Keating, B. G., Kovac, J., Kirby, E., ... Zemcov, M. (2009). QUaD: A high-resolution cosmic microwave background polarimeter. Astrophysical Journal, 692(2), 1221-1246. https://doi.org/10.1088/0004-637X/692/2/1221

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title = "QUaD: A high-resolution cosmic microwave background polarimeter",

abstract = "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 35, 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.",

keywords = "cosmic microwave background, instrumentation: polarimeters",

author = "Hinderks, \{J. R.\} and P. Ade and J. Bock and M. Bowden and Brown, \{M. L.\} and G. Cahill and Carlstrom, \{J. E.\} and Castro, \{P. G.\} and S. Church and T. Culverhouse and R. Friedman and K. Ganga and Gear, \{W. K.\} and S. Gupta and J. Harris and V. Haynes and Keating, \{B. G.\} and J. Kovac and E. Kirby and Lange, \{A. E.\} and E. Leitch and Mallie, \{O. E.\} and S. Melhuish and Y. Memari and A. Murphy and A. Orlando and R. Schwarz and C. O'Sullivan and L. Piccirillo and C. Pryke and N. Rajguru and B. Rusholme and Taylor, \{A. N.\} and Thompson, \{K. L.\} and C. Tucker and Turner, \{A. H.\} and Wu, \{E. Y.S.\} and M. Zemcov",

year = "2009",

month = feb,

day = "20",

doi = "10.1088/0004-637X/692/2/1221",

language = "English",

volume = "692",

pages = "1221--1246",

journal = "Astrophysical Journal",

issn = "0004-637X",

publisher = "American Astronomical Society",

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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, BG, Kovac, J, Kirby, E, Lange, AE, Leitch, E, Mallie, OE, Melhuish, S, Memari, Y, Murphy, A, Orlando, A, Schwarz, R, O'Sullivan, C, Piccirillo, L, Pryke, C, Rajguru, N, Rusholme, B, Taylor, AN, Thompson, KL, Tucker, C, Turner, AH, Wu, EYS & Zemcov, M 2009, 'QUaD: A high-resolution cosmic microwave background polarimeter', Astrophysical Journal, vol. 692, no. 2, pp. 1221-1246. https://doi.org/10.1088/0004-637X/692/2/1221

TY - JOUR

T1 - QUaD

T2 - A high-resolution cosmic microwave background polarimeter

AU - Hinderks, J. R.

AU - Ade, P.

AU - Bock, J.

AU - Bowden, M.

AU - Brown, M. L.

AU - Cahill, G.

AU - Carlstrom, J. E.

AU - Castro, P. G.

AU - Church, S.

AU - Culverhouse, T.

AU - Friedman, R.

AU - Ganga, K.

AU - Gear, W. K.

AU - Gupta, S.

AU - Harris, J.

AU - Haynes, V.

AU - Keating, B. G.

AU - Kovac, J.

AU - Kirby, E.

AU - Lange, A. E.

AU - Leitch, E.

AU - Mallie, O. E.

AU - Melhuish, S.

AU - Memari, Y.

AU - Murphy, A.

AU - Orlando, A.

AU - Schwarz, R.

AU - O'Sullivan, C.

AU - Piccirillo, L.

AU - Pryke, C.

AU - Rajguru, N.

AU - Rusholme, B.

AU - Taylor, A. N.

AU - Thompson, K. L.

AU - Tucker, C.

AU - Turner, A. H.

AU - Wu, E. Y.S.

AU - Zemcov, M.

PY - 2009/2/20

Y1 - 2009/2/20

N2 - 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 35, 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.

AB - 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 35, 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.

KW - cosmic microwave background

KW - instrumentation: polarimeters

UR - https://www.scopus.com/pages/publications/67549106279

U2 - 10.1088/0004-637X/692/2/1221

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

M3 - Article

SN - 0004-637X

VL - 692

SP - 1221

EP - 1246

JO - Astrophysical Journal

JF - Astrophysical Journal

IS - 2

ER -

QUaD: A high-resolution cosmic microwave background polarimeter

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Keywords

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