MEASUREMENTS OF E-MODE POLARIZATION AND TEMPERATURE-E-MODE CORRELATION IN THE COSMIC MICROWAVE BACKGROUND FROM 100 SQUARE DEGREES OF SPTPOL DATA

A. T. Crites; J. W. Henning; P. A R Ade; K. A. Aird; J. E. Austermann; J. A. Beall; A. N. Bender; B. A. Benson; L. E. Bleem; J. E. Carlstrom; C. L. Chang; H. C. Chiang; H. M. Cho; R. Citron; T. M. Crawford; T. De Haan; M. A. Dobbs; W. Everett; J. Gallicchio; J. Gao; E. M. George; A. Gilbert; N. W. Halverson; D. Hanson; N. Harrington; G. C. Hilton; G. P. Holder; W. L. Holzapfel; S. Hoover; Z. Hou; J. D. Hrubes; N. Huang; J. Hubmayr; K. D. Irwin; R. Keisler; L. Knox; A. T. Lee; E. M. Leitch; D. Li; C. Liang; D. Luong-Van; J. J. McMahon; J. Mehl; S. S. Meyer; L. Mocanu; T. E. Montroy; T. Natoli; J. P. Nibarger; V. Novosad; S. Padin; C. Pryke; C. L. Reichardt; J. E. Ruhl; B. R. Saliwanchik; J. T. Sayre; K. K. Schaffer; G. Smecher; A. A. Stark; K. T. Story; C. Tucker; K. Vanderlinde; J. D. Vieira; G. Wang; N. Whitehorn; V. Yefremenko; O. Zahn

doi:10.1088/0004-637X/805/1/36

MEASUREMENTS OF E-MODE POLARIZATION AND TEMPERATURE-E-MODE CORRELATION IN THE COSMIC MICROWAVE BACKGROUND FROM 100 SQUARE DEGREES OF SPTPOL DATA

A. T. Crites
, J. W. Henning
, P. A R Ade
, K. A. Aird
, J. E. Austermann
, J. A. Beall
, A. N. Bender
, B. A. Benson
, L. E. Bleem
, J. E. Carlstrom
, C. L. Chang
, H. C. Chiang
, H. M. Cho
, R. Citron
, T. M. Crawford
, T. De Haan
, M. A. Dobbs
, W. Everett
, J. Gallicchio
, J. Gao

E. M. George, A. Gilbert, N. W. Halverson, D. Hanson, N. Harrington, G. C. Hilton, G. P. Holder, W. L. Holzapfel, S. Hoover, Z. Hou, J. D. Hrubes, N. Huang, J. Hubmayr, K. D. Irwin, R. Keisler, L. Knox, A. T. Lee, E. M. Leitch, D. Li, C. Liang, D. Luong-Van, J. J. McMahon, J. Mehl, S. S. Meyer, L. Mocanu, T. E. Montroy, T. Natoli, J. P. Nibarger, V. Novosad, S. Padin, C. Pryke, C. L. Reichardt, J. E. Ruhl, B. R. Saliwanchik, J. T. Sayre, K. K. Schaffer, G. Smecher, A. A. Stark, K. T. Story, C. Tucker, K. Vanderlinde, J. D. Vieira, G. Wang, N. Whitehorn, V. Yefremenko, O. Zahn

Physics and Astronomy (Twin Cities)

Research output: Contribution to journal › Article › peer-review

62 Scopus citations

Abstract

We present measurements of E-mode polarization and temperature-E-mode correlation in the cosmic microwave background using data from the first season of observations with SPTpol, the polarization-sensitive receiver currently installed on the South Pole Telescope (SPT). The observations used in this work cover 100 deg² of sky with arcminute resolution at 150 GHz. We report the E-mode angular auto-power spectrum (EE) and the temperature-E-mode angular cross-power spectrum (TE) over the multipole range 500 < ℓ ≤ 5000. These power spectra improve on previous measurements in the high-ℓ (small-scale) regime. We fit the combination of the SPTpol power spectra, data from Planck, and previous SPT measurements with a six-parameter ΛCDM cosmological model. We find that the best-fit parameters are consistent with previous results. The improvement in high-ℓ sensitivity over previous measurements leads to a significant improvement in the limit on polarized point-source power: after masking sources brighter than 50 mJy in unpolarized flux at 150 GHz, we find a 95% confidence upper limit on unclustered point-source power in the EE spectrum of D_ℓ = ℓ(ℓ + ℓ)C_ℓ/2π < 0.40 μK² at ℓ = 3000, indicating that future EE measurements will not be limited by power from unclustered point sources in the multipole range , and possibly much higher in ℓ.

Original language	English (US)
Article number	36
Journal	Astrophysical Journal
Volume	805
Issue number	1
DOIs	https://doi.org/10.1088/0004-637X/805/1/36
State	Published - May 20 2015

Bibliographical note

Publisher Copyright:
© 2015. The American Astronomical Society. All rights reserved.

Keywords

Cosmic background radiation
Cosmology: observations
Polarization

Publisher link

10.1088/0004-637X/805/1/36

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Crites, A. T., Henning, J. W., Ade, P. A. R., Aird, K. A., Austermann, J. E., Beall, J. A., Bender, A. N., Benson, B. A., Bleem, L. E., Carlstrom, J. E., Chang, C. L., Chiang, H. C., Cho, H. M., Citron, R., Crawford, T. M., Haan, T. D., Dobbs, M. A., Everett, W., Gallicchio, J., ... Zahn, O. (2015). MEASUREMENTS OF E-MODE POLARIZATION AND TEMPERATURE-E-MODE CORRELATION IN THE COSMIC MICROWAVE BACKGROUND FROM 100 SQUARE DEGREES OF SPTPOL DATA. Astrophysical Journal, 805(1), Article 36. https://doi.org/10.1088/0004-637X/805/1/36

Crites, AT, Henning, JW, Ade, PAR, Aird, KA, Austermann, JE, Beall, JA, Bender, AN, Benson, BA, Bleem, LE, Carlstrom, JE, Chang, CL, Chiang, HC, Cho, HM, Citron, R, Crawford, TM, Haan, TD, Dobbs, MA, Everett, W, Gallicchio, J, Gao, J, George, EM, Gilbert, A, Halverson, NW, Hanson, D, Harrington, N, Hilton, GC, Holder, GP, Holzapfel, WL, Hoover, S, Hou, Z, Hrubes, JD, Huang, N, Hubmayr, J, Irwin, KD, Keisler, R, Knox, L, Lee, AT, Leitch, EM, Li, D, Liang, C, Luong-Van, D, McMahon, JJ, Mehl, J, Meyer, SS, Mocanu, L, Montroy, TE, Natoli, T, Nibarger, JP, Novosad, V, Padin, S, Pryke, C, Reichardt, CL, Ruhl, JE, Saliwanchik, BR, Sayre, JT, Schaffer, KK, Smecher, G, Stark, AA, Story, KT, Tucker, C, Vanderlinde, K, Vieira, JD, Wang, G, Whitehorn, N, Yefremenko, V & Zahn, O 2015, 'MEASUREMENTS OF E-MODE POLARIZATION AND TEMPERATURE-E-MODE CORRELATION IN THE COSMIC MICROWAVE BACKGROUND FROM 100 SQUARE DEGREES OF SPTPOL DATA', Astrophysical Journal, vol. 805, no. 1, 36. https://doi.org/10.1088/0004-637X/805/1/36

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title = "MEASUREMENTS OF E-MODE POLARIZATION AND TEMPERATURE-E-MODE CORRELATION IN THE COSMIC MICROWAVE BACKGROUND FROM 100 SQUARE DEGREES OF SPTPOL DATA",

abstract = "We present measurements of E-mode polarization and temperature-E-mode correlation in the cosmic microwave background using data from the first season of observations with SPTpol, the polarization-sensitive receiver currently installed on the South Pole Telescope (SPT). The observations used in this work cover 100 deg2 of sky with arcminute resolution at 150 GHz. We report the E-mode angular auto-power spectrum (EE) and the temperature-E-mode angular cross-power spectrum (TE) over the multipole range 500 < ℓ ≤ 5000. These power spectra improve on previous measurements in the high-ℓ (small-scale) regime. We fit the combination of the SPTpol power spectra, data from Planck, and previous SPT measurements with a six-parameter ΛCDM cosmological model. We find that the best-fit parameters are consistent with previous results. The improvement in high-ℓ sensitivity over previous measurements leads to a significant improvement in the limit on polarized point-source power: after masking sources brighter than 50 mJy in unpolarized flux at 150 GHz, we find a 95\% confidence upper limit on unclustered point-source power in the EE spectrum of Dℓ = ℓ(ℓ + ℓ)Cℓ/2π < 0.40 μK2 at ℓ = 3000, indicating that future EE measurements will not be limited by power from unclustered point sources in the multipole range , and possibly much higher in ℓ.",

keywords = "Cosmic background radiation, Cosmology: observations, Polarization",

author = "Crites, \{A. T.\} and Henning, \{J. W.\} and Ade, \{P. A R\} and Aird, \{K. A.\} and Austermann, \{J. E.\} and Beall, \{J. A.\} and Bender, \{A. N.\} and Benson, \{B. A.\} and Bleem, \{L. E.\} and Carlstrom, \{J. E.\} and Chang, \{C. L.\} and Chiang, \{H. C.\} and Cho, \{H. M.\} and R. Citron and Crawford, \{T. M.\} and Haan, \{T. De\} and Dobbs, \{M. A.\} and W. Everett and J. Gallicchio and J. Gao and George, \{E. M.\} and A. Gilbert and Halverson, \{N. W.\} and D. Hanson and N. Harrington and Hilton, \{G. C.\} and Holder, \{G. P.\} and Holzapfel, \{W. L.\} and S. Hoover and Z. Hou and Hrubes, \{J. D.\} and N. Huang and J. Hubmayr and Irwin, \{K. D.\} and R. Keisler and L. Knox and Lee, \{A. T.\} and Leitch, \{E. M.\} and D. Li and C. Liang and D. Luong-Van and McMahon, \{J. J.\} and J. Mehl and Meyer, \{S. S.\} and L. Mocanu and Montroy, \{T. E.\} and T. Natoli and Nibarger, \{J. P.\} and V. Novosad and S. Padin and C. Pryke and Reichardt, \{C. L.\} and Ruhl, \{J. E.\} and Saliwanchik, \{B. R.\} and Sayre, \{J. T.\} and Schaffer, \{K. K.\} and G. Smecher and Stark, \{A. A.\} and Story, \{K. T.\} and C. Tucker and K. Vanderlinde and Vieira, \{J. D.\} and G. Wang and N. Whitehorn and V. Yefremenko and O. Zahn",

year = "2015",

month = may,

day = "20",

doi = "10.1088/0004-637X/805/1/36",

language = "English (US)",

volume = "805",

journal = "Astrophysical Journal",

issn = "0004-637X",

publisher = "American Astronomical Society",

number = "1",

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TY - JOUR

T1 - MEASUREMENTS OF E-MODE POLARIZATION AND TEMPERATURE-E-MODE CORRELATION IN THE COSMIC MICROWAVE BACKGROUND FROM 100 SQUARE DEGREES OF SPTPOL DATA

AU - Crites, A. T.

AU - Henning, J. W.

AU - Ade, P. A R

AU - Aird, K. A.

AU - Austermann, J. E.

AU - Beall, J. A.

AU - Bender, A. N.

AU - Benson, B. A.

AU - Bleem, L. E.

AU - Carlstrom, J. E.

AU - Chang, C. L.

AU - Chiang, H. C.

AU - Cho, H. M.

AU - Citron, R.

AU - Crawford, T. M.

AU - Haan, T. De

AU - Dobbs, M. A.

AU - Everett, W.

AU - Gallicchio, J.

AU - Gao, J.

AU - George, E. M.

AU - Gilbert, A.

AU - Halverson, N. W.

AU - Hanson, D.

AU - Harrington, N.

AU - Hilton, G. C.

AU - Holder, G. P.

AU - Holzapfel, W. L.

AU - Hoover, S.

AU - Hou, Z.

AU - Hrubes, J. D.

AU - Huang, N.

AU - Hubmayr, J.

AU - Irwin, K. D.

AU - Keisler, R.

AU - Knox, L.

AU - Lee, A. T.

AU - Leitch, E. M.

AU - Li, D.

AU - Liang, C.

AU - Luong-Van, D.

AU - McMahon, J. J.

AU - Mehl, J.

AU - Meyer, S. S.

AU - Mocanu, L.

AU - Montroy, T. E.

AU - Natoli, T.

AU - Nibarger, J. P.

AU - Novosad, V.

AU - Padin, S.

AU - Pryke, C.

AU - Reichardt, C. L.

AU - Ruhl, J. E.

AU - Saliwanchik, B. R.

AU - Sayre, J. T.

AU - Schaffer, K. K.

AU - Smecher, G.

AU - Stark, A. A.

AU - Story, K. T.

AU - Tucker, C.

AU - Vanderlinde, K.

AU - Vieira, J. D.

AU - Wang, G.

AU - Whitehorn, N.

AU - Yefremenko, V.

AU - Zahn, O.

PY - 2015/5/20

Y1 - 2015/5/20

N2 - We present measurements of E-mode polarization and temperature-E-mode correlation in the cosmic microwave background using data from the first season of observations with SPTpol, the polarization-sensitive receiver currently installed on the South Pole Telescope (SPT). The observations used in this work cover 100 deg2 of sky with arcminute resolution at 150 GHz. We report the E-mode angular auto-power spectrum (EE) and the temperature-E-mode angular cross-power spectrum (TE) over the multipole range 500 < ℓ ≤ 5000. These power spectra improve on previous measurements in the high-ℓ (small-scale) regime. We fit the combination of the SPTpol power spectra, data from Planck, and previous SPT measurements with a six-parameter ΛCDM cosmological model. We find that the best-fit parameters are consistent with previous results. The improvement in high-ℓ sensitivity over previous measurements leads to a significant improvement in the limit on polarized point-source power: after masking sources brighter than 50 mJy in unpolarized flux at 150 GHz, we find a 95% confidence upper limit on unclustered point-source power in the EE spectrum of Dℓ = ℓ(ℓ + ℓ)Cℓ/2π < 0.40 μK2 at ℓ = 3000, indicating that future EE measurements will not be limited by power from unclustered point sources in the multipole range , and possibly much higher in ℓ.

AB - We present measurements of E-mode polarization and temperature-E-mode correlation in the cosmic microwave background using data from the first season of observations with SPTpol, the polarization-sensitive receiver currently installed on the South Pole Telescope (SPT). The observations used in this work cover 100 deg2 of sky with arcminute resolution at 150 GHz. We report the E-mode angular auto-power spectrum (EE) and the temperature-E-mode angular cross-power spectrum (TE) over the multipole range 500 < ℓ ≤ 5000. These power spectra improve on previous measurements in the high-ℓ (small-scale) regime. We fit the combination of the SPTpol power spectra, data from Planck, and previous SPT measurements with a six-parameter ΛCDM cosmological model. We find that the best-fit parameters are consistent with previous results. The improvement in high-ℓ sensitivity over previous measurements leads to a significant improvement in the limit on polarized point-source power: after masking sources brighter than 50 mJy in unpolarized flux at 150 GHz, we find a 95% confidence upper limit on unclustered point-source power in the EE spectrum of Dℓ = ℓ(ℓ + ℓ)Cℓ/2π < 0.40 μK2 at ℓ = 3000, indicating that future EE measurements will not be limited by power from unclustered point sources in the multipole range , and possibly much higher in ℓ.

KW - Cosmic background radiation

KW - Cosmology: observations

KW - Polarization

UR - https://www.scopus.com/pages/publications/84929994710

UR - https://www.scopus.com/pages/publications/84929994710#tab=citedBy

U2 - 10.1088/0004-637X/805/1/36

DO - 10.1088/0004-637X/805/1/36

M3 - Article

AN - SCOPUS:84929994710

SN - 0004-637X

VL - 805

JO - Astrophysical Journal

JF - Astrophysical Journal

IS - 1

M1 - 36

ER -

MEASUREMENTS OF E-MODE POLARIZATION AND TEMPERATURE-E-MODE CORRELATION IN THE COSMIC MICROWAVE BACKGROUND FROM 100 SQUARE DEGREES OF SPTPOL DATA

Abstract

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Keywords

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