Journal of Low Temperature Physics

, Volume 167, Issue 5, pp 859–864

An Overview of the SPTpol Experiment

  • L. Bleem
  • P. Ade
  • K. Aird
  • J. Austermann
  • J. Beall
  • D. Becker
  • B. Benson
  • J. Britton
  • J. Carlstrom
  • C. L. Chang
  • H. Cho
  • T. de Haan
  • T. Crawford
  • A. Crites
  • A. Datesman
  • M. Dobbs
  • W. Everett
  • A. Ewall-Wice
  • E. George
  • N. Halverson
  • N. Harrington
  • J. Henning
  • G. Hilton
  • W. Holzapfel
  • S. Hoover
  • J. Hubmayr
  • K. Irwin
  • R. Keisler
  • J. Kennedy
  • A. Lee
  • E. Leitch
  • D. Li
  • M. Lueker
  • D. P. Marrone
  • J. McMahon
  • J. Mehl
  • S. Meyer
  • J. Montgomery
  • T. Montroy
  • T. Natoli
  • J. Nibarger
  • M. Niemack
  • V. Novosad
  • S. Padin
  • C. Pryke
  • C. Reichardt
  • J. Ruhl
  • B. Saliwanchik
  • J. Sayre
  • K. Schafer
  • E. Shirokoff
  • K. Story
  • K. Vanderlinde
  • J. Vieira
  • G. Wang
  • R. Williamson
  • V. Yefremenko
  • K. W. Yoon
  • E. Young
Article

DOI: 10.1007/s10909-012-0505-y

Cite this article as:
Bleem, L., Ade, P., Aird, K. et al. J Low Temp Phys (2012) 167: 859. doi:10.1007/s10909-012-0505-y

Abstract

In 2012 the South Pole Telescope (SPT) will begin a 625 deg2 survey to measure the polarization anisotropy of the cosmic microwave background (CMB). Observations of the CMB B-mode angular power spectrum will be used to search for the large angular scale signal induced by inflationary gravitational waves. Additionally, the B-mode spectrum will enable a measurement of the neutrino mass through the gravitational lensing of the CMB. The new 780 pixel polarization-sensitive camera is composed of two different detector architectures and will map the sky at two frequencies. At 150 GHz, the camera consists of arrays of corrugated feedhorn-coupled TES polarimeters fabricated at the National Institute of Standards and Technology (NIST). At 90 GHz, we use individually packaged dual-polarization absorber-coupled polarimeters developed at Argonne National Laboratory. Each 90 GHz pixel couples to the telescope through machined contoured feedhorns. The entire focal plane is read out using a digital frequency-domain multiplexer system. We discuss the design and goals of this experiment and provide a description of the detectors.

Keywords

PolarimetryTransition-edge sensorsBolometersCosmic microwave backgroundCosmology

Copyright information

© Springer Science+Business Media, LLC 2012

Authors and Affiliations

  • L. Bleem
    • 1
  • P. Ade
    • 2
  • K. Aird
    • 1
  • J. Austermann
    • 3
  • J. Beall
    • 4
  • D. Becker
    • 4
  • B. Benson
    • 1
  • J. Britton
    • 4
  • J. Carlstrom
    • 1
    • 5
  • C. L. Chang
    • 1
    • 5
  • H. Cho
    • 4
  • T. de Haan
    • 6
  • T. Crawford
    • 1
  • A. Crites
    • 1
  • A. Datesman
    • 7
  • M. Dobbs
    • 6
  • W. Everett
    • 1
  • A. Ewall-Wice
    • 1
  • E. George
    • 8
  • N. Halverson
    • 3
  • N. Harrington
    • 8
  • J. Henning
    • 3
  • G. Hilton
    • 4
  • W. Holzapfel
    • 8
  • S. Hoover
    • 1
  • J. Hubmayr
    • 4
  • K. Irwin
    • 4
  • R. Keisler
    • 1
  • J. Kennedy
    • 6
  • A. Lee
    • 8
  • E. Leitch
    • 1
  • D. Li
    • 4
  • M. Lueker
    • 9
  • D. P. Marrone
    • 15
  • J. McMahon
    • 10
  • J. Mehl
    • 1
  • S. Meyer
    • 1
  • J. Montgomery
    • 1
  • T. Montroy
    • 12
  • T. Natoli
    • 1
  • J. Nibarger
    • 4
  • M. Niemack
    • 4
  • V. Novosad
    • 7
  • S. Padin
    • 9
  • C. Pryke
    • 11
  • C. Reichardt
    • 8
  • J. Ruhl
    • 12
  • B. Saliwanchik
    • 12
  • J. Sayre
    • 12
  • K. Schafer
    • 13
  • E. Shirokoff
    • 9
  • K. Story
    • 1
  • K. Vanderlinde
    • 6
  • J. Vieira
    • 9
  • G. Wang
    • 7
  • R. Williamson
    • 1
  • V. Yefremenko
    • 7
  • K. W. Yoon
    • 14
  • E. Young
    • 8
  1. 1.Kavli Institute for Cosmological Physics, Department of Physics, Enrico Fermi InstituteThe University of ChicagoChicagoUSA
  2. 2.Cardiff School of Physics and AstronomyCardiff UniversityCardiffUK
  3. 3.Department of Astrophysical and Planetary SciencesUniversity of ColoradoBoulderUSA
  4. 4.NISTBoulderUSA
  5. 5.Argonne National Laboratory—HEP DivisionArgonneUSA
  6. 6.McGill UniversityMontrealCanada
  7. 7.Argonne National Laboratory—MSDArgonneUSA
  8. 8.University of CaliforniaBerkeleyUSA
  9. 9.California Institute of TechnologyPasadenaUSA
  10. 10.University of MichiganAnn ArborUSA
  11. 11.University of MinnesotaMinneapolisUSA
  12. 12.Case Western Reserve UniversityClevelandUSA
  13. 13.School of the Art Institute of ChicagoChicagoUSA
  14. 14.Stanford UniversityPalo AltoUSA
  15. 15.Steward ObservatoryUniversity of ArizonaTucsonUSA