CaltechAUTHORS
  A Caltech Library Service

QUaD: A High-Resolution Cosmic Microwave Background Polarimeter

Hinderks, J. R. and Ade, P. and Bock, J. and Bowden, M. and Brown, M. L. and Cahill, G. and Carlstrom, J. E. and Castro, P. G. and Church, S. and Culverhouse, T. and Friedman, R. and Ganga, K. and Gear, W. K. and Gupta, S. and Harris, J. and Haynes, V. and Keating, B. G. and Kovac, J. and Kirby, E. and Lange, A. E. and Leitch, E. and Mallie, O. E. and Melhuish, S. and Memari, Y. and Murphy, A. and Orlando, A. and Schwarz, R. and O'Sullivan, C. and Piccirillo, L. and Pryke, C. and Rajguru, N. and Rusholme, B. and Taylor, A. N. and Thompson, K. L. and Tucker, C. and Turner, A. H. and Wu, E. Y. S. and Zemcov, M. (2009) QUaD: A High-Resolution Cosmic Microwave Background Polarimeter. Astrophysical Journal, 692 (2). pp. 1221-1246. ISSN 0004-637X. https://resolver.caltech.edu/CaltechAUTHORS:20090831-141710879

[img]
Preview
PDF - Published Version
See Usage Policy.

2584Kb

Use this Persistent URL to link to this item: https://resolver.caltech.edu/CaltechAUTHORS:20090831-141710879

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.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1088/0004-637X/692/2/1221DOIArticle
http://www.iop.org/EJ/abstract/0004-637X/692/2/1221/PublisherArticle
ORCID:
AuthorORCID
Bock, J.0000-0002-5710-5212
Carlstrom, J. E.0000-0002-2044-7665
Kirby, E.0000-0001-6196-5162
Rusholme, B.0000-0001-7648-4142
Zemcov, M.0000-0001-8253-1451
Additional Information:© 2009 The American Astronomical Society. Received 2008 May 14; accepted 2008 October 2; published 2009 February 24. We acknowledge the staff of the Amundsen-Scott South Pole Station and all involved in the United States Antarctic Program for their superb support during the construction and operation of this experiment. Special thanks go to our brave winter-over scientist Robert Schwarzwho has spent three consecutivewinter seasons with the QUaD. We also acknowledge the tremendous efforts of the Stanford University Physics Department machine shop in the construction of the focal plane assembly. J.R.H. thanks David Chuss for useful comments on this draft and Simon Radford for providing the 350 μm tipper data. QUaD is funded by the National Science Foundation in the USA, through grants AST-0096778,ANT-0338138,ANT-0338335, and ANT- 0338238, by the UK Science and technology Facilities Council (STFC) and its predecessor the Particle Physics and Astronomy Research Council (PPARC), and by the Science Foundation Ireland. J.R.H. acknowledges the support of an NSF Graduate Research Fellowship, a Stanford Graduate Fellowship, and a NASA Postdoctoral Fellowship. M.L.B. and A.O. acknowledge the award of PPARC fellowships. P.G.C. is funded by the Fundação para a Ciência e a Tecnologia. S.E.C. acknowledges support from a Stanford Terman Fellowship. J.M.K. acknowledges support from a John B. and Nelly L. Kilroy Foundation Fellowship. C.P. and J.E.C. acknowledge partial support from the Kavli Institute for Cosmological Physics through the grant NSF PHY-0114422. E.Y.W. acknowledges receipt of an NDSEG fellowship. M.Z. acknowledges the support of a NASA Postdoctoral Fellowship. This research was supported in part by appointments to the NASA Postdoctoral Program at the Goddard Space Flight Center (J.R.H.) and the Jet Propulsion Laboratory (M.Z.), administered by Oak Ridge Associated Universities through a contract with NASA.
Funders:
Funding AgencyGrant Number
NSFAST-0096778
NSFANT-0338138
NSFANT-0338335
NSFANT-0338238
Science and Technology Facilities Council (STFC)UNSPECIFIED
Particle Physics and Astronomy Research Council (PPARC)UNSPECIFIED
Science Foundation IrelandUNSPECIFIED
NSF Graduate Research FellowshipUNSPECIFIED
Stanford Graduate FellowshipUNSPECIFIED
NASA Postdoctoral FellowshipUNSPECIFIED
Fundação para a Ciência e a TecnologiaUNSPECIFIED
Stanford Terman FellowshipUNSPECIFIED
John B. and Nelly L. Kilroy FoundationUNSPECIFIED
NSFPHY-0114422
Kavli Institute for Cosmological PhysicsUNSPECIFIED
Subject Keywords:cosmic microwave background; instrumentation: polarimeters
Issue or Number:2
Record Number:CaltechAUTHORS:20090831-141710879
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20090831-141710879
Official Citation: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, and M. Zemcov 2009 ApJ 692 1221-1246 doi: 10.1088/0004-637X/692/2/1221
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:15497
Collection:CaltechAUTHORS
Deposited By: Ruth Sustaita
Deposited On:11 Sep 2009 22:32
Last Modified:09 Mar 2020 13:19

Repository Staff Only: item control page