Measurements of Sub-degree B-mode Polarization in the Cosmic Microwave Background from 100 Square Degrees of SPTpol Data

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

doi:10.1088/0004-637X/807/2/151

Title: Measurements of Sub-degree B-mode Polarization in the Cosmic Microwave Background from 100 Square Degrees of SPTpol Data

Abstract

We present a measurement of the $$B$$-mode polarization power spectrum (the $BB$ spectrum) from 100 $$\mathrm{deg}^2$$ of sky observed with SPTpol, a polarization-sensitive receiver currently installed on the South Pole Telescope. The observations used in this work were taken during 2012 and early 2013 and include data in spectral bands centered at 95 and 150 GHz. We report the $BB$ spectrum in five bins in multipole space, spanning the range $$300 \le \ell \le 2300$$, and for three spectral combinations: 95 GHz $$\times$$ 95 GHz, 95 GHz $$\times$$ 150 GHz, and 150 GHz $$\times$$ 150 GHz. We subtract small ($$< 0.5 \sigma$$ in units of statistical uncertainty) biases from these spectra and account for the uncertainty in those biases. The resulting power spectra are inconsistent with zero power but consistent with predictions for the $BB$ spectrum arising from the gravitational lensing of $$E$$-mode polarization. If we assume no other source of $BB$ power besides lensed $$B$$ modes, we determine a preference for lensed $$B$$ modes of $$4.9 \sigma$$. After marginalizing over tensor power and foregrounds, namely polarized emission from galactic dust and extragalactic sources, this significance is $$4.3 \sigma$$. Fitting for a single parameter, $$A_\mathrm{lens}$$, that multiplies the predicted lensed $$B$$-mode spectrum, and marginalizing over tensor power and foregrounds, we find $$A_\mathrm{lens} = 1.08 \pm 0.26$$, indicating that our measured spectra are consistent with the signal expected from gravitational lensing. The data presented here provide the best measurement to date of the $$B$$-mode power spectrum on these angular scales.

Authors:

Keisler, R. ^[1]; Hoover, S. ^[2]; Harrington, N. ^[3]; Henning, J. W. ^[4]; Ade, P. A. R. ^[5]; Aird, K. A. ^[6]; Austermann, J. E. ^[7]; Beall, J. A. ^[8]; Bender, A. N. ^[9]; Benson, B. A. ^[10]; Bleem, L. E. ^[11]; Carlstrom, J. E. ^[12]; Chang, C. L. ^[13]; Chiang, H. C. ^[14]; Cho, H-M. ^[15]; Citron, R. ^[16]; Crawford, T. M. ^[17]; Crites, A. T. ^[18]; de Haan, T. ^[3]; Dobbs, M. A. ^[19] more »

Stanford Univ., CA (United States). Dept. of Physics; Stanford Univ., CA (United States). Kavli Inst. for Particle Astrophysics and Cosmology
Univ. of Chicago, IL (United States). Kavli Inst. for Cosmological Physics (KICP); Univ. of Chicago, IL (United States). Dept. of Physics
Univ. of California, Berkeley, CA (United States). Dept. of Physics
Univ. of Chicago, IL (United States). Kavli Inst. for Cosmological Physics (KICP); Univ. of Colorado, Boulder, CO (United States). Dept. of Astrophysical and Planetary Sciences
Cardiff Univ. (United Kingdom). School of Physics and Astronomy
Univ. of Chicago, IL (United States)
Univ. of Colorado, Boulder, CO (United States). Dept. of Astrophysical and Planetary Sciences; National Inst. of Standards and Technology (NIST), Boulder, CO (United States). NIST Quantum Devices Group
National Inst. of Standards and Technology (NIST), Boulder, CO (United States). NIST Quantum Devices Group
Univ. of Chicago, IL (United States). Kavli Inst. for Cosmological Physics (KICP); McGill Univ., Montreal, QC (Canada). Dept of Physics; Argonne National Lab. (ANL), Argonne, IL (United States). High Energy Physics Division
Univ. of Chicago, IL (United States). Kavli Inst. for Cosmological Physics (KICP); Univ. of Chicago, IL (United States). Dept. of Astronomy and Astrophysics; Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States)
Univ. of Chicago, IL (United States). Kavli Inst. for Cosmological Physics (KICP); Univ. of Chicago, IL (United States). Dept of Physics; Argonne National Lab. (ANL), Argonne, IL (United States). High Energy Physics Division
Univ. of Chicago, IL (United States). Kavli Inst. for Cosmological Physics (KICP); Univ. of Chicago, IL (United States). Dept of Physics; Argonne National Lab. (ANL), Argonne, IL (United States). High Energy Physics Division; Univ. of Chicago, IL (United States). Dept. of Astronomy and Astrophysics; Univ. of Chicago, IL (United States). Enrico Fermi Inst.
Univ. of Chicago, IL (United States). Kavli Inst. for Cosmological Physics (KICP); Argonne National Lab. (ANL), Argonne, IL (United States). High Energy Physics Division; Univ. of Chicago, IL (United States). Dept. Astronomy and Astrophysics
Univ. of KwaZulu-Natal, Durban (South Africa). School of Mathematics, Statistics & Computer Science
SLAC National Accelerator Lab., Menlo Park, CA (United States)
Univ. of Chicago, IL (United States). Kavli Inst. for Cosmological Physics
Univ. of Chicago, IL (United States). Kavli Inst. for Cosmological Physics (KICP); Univ. of Chicago, IL (United States). Dept. of Astronomy and Astrophysics
Univ. of Chicago, IL (United States). Kavli Inst. for Cosmological Physics (KICP); Univ. of Chicago, IL (United States). Dept. of Astronomy and Astrophysics; California Inst. of Technology (CalTech), Pasadena, CA (United States)
McGill Univ., Montreal, QC (Canada). Dept of Physics; Canadian Inst. for Advanced Research, Toronto, ON (Canada). CIFAR Program in Cosmology and Gravity
Univ. of Colorado, Boulder, CO (United States). Dept. of Astrophysical and Planetary Sciences
McGill Univ., Montreal, QC (Canada). Dept of Physics
Univ. of Colorado, Boulder, CO (United States). Dept. of Astrophysical and Planetary Sciences; Univ. of Colorado, Boulder, CO (United States). Dept. of Physics
Stanford Univ., CA (United States). Dept. of Physics; SLAC National Accelerator Lab., Menlo Park, CA (United States)
Univ. of California, Davis, CA (United States). Dept. of Physics
Univ. of California, Berkeley, CA (United States). Dept. of Physics; Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States). Physics Division
National Inst. of Standards and Technology (NIST), Boulder, CO (United States). NIST Quantum Devices Group; SLAC National Accelerator Lab., Menlo Park, CA (United States)
Univ. of Arizona, Tucson, AZ (United States). Steward Observatory
Univ. of Michigan, Ann Arbor, MI (United States). Dept. of Physics
Univ. of Chicago, IL (United States). Kavli Inst. for Cosmological Physics (KICP); Argonne National Lab. (ANL), Argonne, IL (United States). High Energy Physics Division
Univ. of Chicago, IL (United States). Kavli Inst. for Cosmological Physics (KICP); Univ. of Chicago, IL (United States). Dept. of Astronomy and Astrophysics; Univ. of Chicago, IL (United States). Dept. of Physics; Univ. of Chicago, IL (United States). Enrico Fermi Inst.
Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States). Materials Sciences Division
California Inst. of Technology (CalTech), Pasadena, CA (United States)
Univ. of Minnesota, Minneapolis, MN (United States). School of Physics and Astronomy
Univ. of California, Berkeley, CA (United States). Dept. of Physics; Univ. of Melbourne (Australia). School of Physics
Case Western Reserve Univ., Cleveland, OH (United States). Center for Education and Research in Cosmology and Astrophysics and Physics Dept.
Univ. of Chicago, IL (United States). Kavli Inst. for Cosmological Physics; Univ. of Chicago, IL (United States). Enrico Fermi Inst.; School of the Art Inst. of Chicago, Chicago, IL (United States). Liberal Arts Dept.
McGill Univ., Montreal, QC (Canada). Dept of Physics; Three-Speed Logic, Inc., Vancouver, BC (Canada)
Harvard-Smithsonian Center for Astrophysics, Cambridge, MA (United States)
Univ. of Toronto, ON (Canada). Dunlap Inst. for Astronomy & Astrophysics; Univ. of Toronto, ON (Canada). Dept. of Astronomy & Astrophysics
Univ. of Illinois, Urbana-Champaign, IL (United States). Astronomy Dept.; Univ. of Illinois, Urbana-Champaign, IL (United States). Dept. of Physics
Argonne National Lab. (ANL), Argonne, IL (United States). High Energy Physics Division
Univ. of California, Berkeley, CA (United States). Berkeley Center for Cosmological Physics, Dept. of Physics; Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States)

Publication Date:: Thu Jul 09 00:00:00 EDT 2015

Research Org.:: Argonne National Lab. (ANL), Argonne, IL (United States); Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States); SLAC National Accelerator Lab., Menlo Park, CA (United States); Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States)

Sponsoring Org.:: USDOE Office of Science (SC), High Energy Physics (HEP); National Science Foundation (NSF); Gordon and Betty Moore Foundation; Natural Sciences and Engineering Research Council of Canada (NSERC); Canadian Institute for Advanced Research

Contributing Org.:: SPT

OSTI Identifier:: 1390209

Alternate Identifier(s):: OSTI ID: 1390207

Report Number(s):: arXiv:1503.02315; FERMILAB-PUB-15-672-AE
Journal ID: ISSN 1538-4357; 1351177

Grant/Contract Number:: AC02-07CH11359; AC02-06CH11357; AC02-05CH11231; PLR-1248097; PHY-0114422; GBMF#947; AST-1402161

Resource Type:: Accepted Manuscript

Journal Name:: The Astrophysical Journal (Online)

Additional Journal Information:: Journal Name: The Astrophysical Journal (Online); Journal Volume: 807; Journal Issue: 2; Journal ID: ISSN 1538-4357

Publisher:: Institute of Physics (IOP)

Country of Publication:: United States

Language:: English

Subject:: 79 ASTRONOMY AND ASTROPHYSICS; cosmic background radiation; cosmology observations

Citation Formats


                    Keisler, R., Hoover, S., Harrington, N., 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., Crites, A. T., de Haan, T., Dobbs, M. A., Everett, W., Gallicchio, J., Gao, J., George, E. M., Gilbert, A., Halverson, N. W., Hanson, D., Hilton, G. C., Holder, G. P., Holzapfel, W. L., Hou, Z., Hrubes, J. D., Huang, N., Hubmayr, J., Irwin, K. D., Knox, L., Lee, A. T., Leitch, E. M., Li, D., Luong-Van, D., Marrone, D. P., McMahon, J. J., Mehl, J., Meyer, S. S., Mocanu, L., Natoli, T., Nibarger, J. P., Novosad, V., Padin, S., Pryke, C., Reichardt, C. L., Ruhl, J. E., Saliwanchik, B. R., Sayre, J. T., Schaffer, K. K., Shirokoff, E., Smecher, G., Stark, A. A., Story, K. T., Tucker, C., Vanderlinde, K., Vieira, J. D., Wang, G., Whitehorn, N., Yefremenko, V., and Zahn, O. Measurements of Sub-degree B-mode Polarization in the Cosmic Microwave Background from 100 Square Degrees of SPTpol Data.  United States: N. p., 2015. 
Web.  doi:10.1088/0004-637X/807/2/151.

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                    Keisler, R., Hoover, S., Harrington, N., 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., Crites, A. T., de Haan, T., Dobbs, M. A., Everett, W., Gallicchio, J., Gao, J., George, E. M., Gilbert, A., Halverson, N. W., Hanson, D., Hilton, G. C., Holder, G. P., Holzapfel, W. L., Hou, Z., Hrubes, J. D., Huang, N., Hubmayr, J., Irwin, K. D., Knox, L., Lee, A. T., Leitch, E. M., Li, D., Luong-Van, D., Marrone, D. P., McMahon, J. J., Mehl, J., Meyer, S. S., Mocanu, L., Natoli, T., Nibarger, J. P., Novosad, V., Padin, S., Pryke, C., Reichardt, C. L., Ruhl, J. E., Saliwanchik, B. R., Sayre, J. T., Schaffer, K. K., Shirokoff, E., Smecher, G., Stark, A. A., Story, K. T., Tucker, C., Vanderlinde, K., Vieira, J. D., Wang, G., Whitehorn, N., Yefremenko, V., & Zahn, O. Measurements of Sub-degree B-mode Polarization in the Cosmic Microwave Background from 100 Square Degrees of SPTpol Data.  United States.  https://doi.org/10.1088/0004-637X/807/2/151

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                    Keisler, R., Hoover, S., Harrington, N., 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., Crites, A. T., de Haan, T., Dobbs, M. A., Everett, W., Gallicchio, J., Gao, J., George, E. M., Gilbert, A., Halverson, N. W., Hanson, D., Hilton, G. C., Holder, G. P., Holzapfel, W. L., Hou, Z., Hrubes, J. D., Huang, N., Hubmayr, J., Irwin, K. D., Knox, L., Lee, A. T., Leitch, E. M., Li, D., Luong-Van, D., Marrone, D. P., McMahon, J. J., Mehl, J., Meyer, S. S., Mocanu, L., Natoli, T., Nibarger, J. P., Novosad, V., Padin, S., Pryke, C., Reichardt, C. L., Ruhl, J. E., Saliwanchik, B. R., Sayre, J. T., Schaffer, K. K., Shirokoff, E., Smecher, G., Stark, A. A., Story, K. T., Tucker, C., Vanderlinde, K., Vieira, J. D., Wang, G., Whitehorn, N., Yefremenko, V., and Zahn, O. Thu .  
"Measurements of Sub-degree B-mode Polarization in the Cosmic Microwave Background from 100 Square Degrees of SPTpol Data".  United States.  https://doi.org/10.1088/0004-637X/807/2/151.  https://www.osti.gov/servlets/purl/1390209.

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@article{osti_1390209,

  title        = {Measurements of Sub-degree B-mode Polarization in the Cosmic Microwave Background from 100 Square Degrees of SPTpol Data},

  author       = {Keisler, R. and Hoover, S. and Harrington, N. 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 Citron, R. and Crawford, T. M. and Crites, A. T. and de Haan, T. and Dobbs, M. A. and Everett, W. and Gallicchio, J. and Gao, J. and George, E. M. and Gilbert, A. and Halverson, N. W. and Hanson, D. and Hilton, G. C. and Holder, G. P. and Holzapfel, W. L. and Hou, Z. and Hrubes, J. D. and Huang, N. and Hubmayr, J. and Irwin, K. D. and Knox, L. and Lee, A. T. and Leitch, E. M. and Li, D. and Luong-Van, D. and Marrone, D. P. and McMahon, J. J. and Mehl, J. and Meyer, S. S. and Mocanu, L. and Natoli, T. and Nibarger, J. P. and Novosad, V. and Padin, S. and Pryke, C. and Reichardt, C. L. and Ruhl, J. E. and Saliwanchik, B. R. and Sayre, J. T. and Schaffer, K. K. and Shirokoff, E. and Smecher, G. and Stark, A. A. and Story, K. T. and Tucker, C. and Vanderlinde, K. and Vieira, J. D. and Wang, G. and Whitehorn, N. and Yefremenko, V. and Zahn, O.},

  abstractNote = {We present a measurement of the $B$-mode polarization power spectrum (the $BB$ spectrum) from 100 $\mathrm{deg}^2$ of sky observed with SPTpol, a polarization-sensitive receiver currently installed on the South Pole Telescope. The observations used in this work were taken during 2012 and early 2013 and include data in spectral bands centered at 95 and 150 GHz. We report the $BB$ spectrum in five bins in multipole space, spanning the range $300 \le \ell \le 2300$, and for three spectral combinations: 95 GHz $\times$ 95 GHz, 95 GHz $\times$ 150 GHz, and 150 GHz $\times$ 150 GHz. We subtract small ($< 0.5 \sigma$ in units of statistical uncertainty) biases from these spectra and account for the uncertainty in those biases. The resulting power spectra are inconsistent with zero power but consistent with predictions for the $BB$ spectrum arising from the gravitational lensing of $E$-mode polarization. If we assume no other source of $BB$ power besides lensed $B$ modes, we determine a preference for lensed $B$ modes of $4.9 \sigma$. After marginalizing over tensor power and foregrounds, namely polarized emission from galactic dust and extragalactic sources, this significance is $4.3 \sigma$. Fitting for a single parameter, $A_\mathrm{lens}$, that multiplies the predicted lensed $B$-mode spectrum, and marginalizing over tensor power and foregrounds, we find $A_\mathrm{lens} = 1.08 \pm 0.26$, indicating that our measured spectra are consistent with the signal expected from gravitational lensing. The data presented here provide the best measurement to date of the $B$-mode power spectrum on these angular scales.},

  doi          = {10.1088/0004-637X/807/2/151},

  journal      = {The Astrophysical Journal (Online)},

  number       = 2,

  volume       = 807,

  place        = {United States},

  year         = {Thu Jul 09 00:00:00 EDT 2015},

  month        = {Thu Jul 09 00:00:00 EDT 2015}

}

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Title: Measurements of Sub-degree B-mode Polarization in the Cosmic Microwave Background from 100 Square Degrees of SPTpol Data

Abstract

Citation Formats

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Neutrino physics from the cosmic microwave background and large scale structure journal, March 2015

The POLARBEAR CMB polarization experiment conference, July 2010

SPTpol: an instrument for CMB polarization measurements with the South Pole Telescope conference, September 2012

Statistical properties of polarized radio sources at high frequency and their impact on cosmic microwave background polarization measurements: Properties of polarized radio sources journal, January 2011

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The 10 Meter South Pole Telescope journal, May 2011

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Inflation Physics from the Cosmic Microwave Background and Large Scale Structure text, January 2013

Neutrino Physics from the Cosmic Microwave Background and Large Scale Structure text, January 2013

Measurements of E-Mode Polarization and Temperature-E-Mode Correlation in the Cosmic Microwave Background from 100 Square Degrees of SPTpol Data text, January 2014

A limit on the detectability of the energy scale of inflation text, January 2002

Separation of Gravitational-Wave and Cosmic-Shear Contributions to Cosmic Microwave Background Polarization text, January 2002

Cosmological parameters from CMB and other data: a Monte-Carlo approach text, January 2002

Unbiased Estimation of an Angular Power Spectrum text, January 2004

HEALPix -- a Framework for High Resolution Discretization, and Fast Analysis of Data Distributed on the Sphere text, January 2004

Statistics of Cosmic Microwave Background Polarization text, January 1996

Gravitational Lensing Effect on Cosmic Microwave Background Polarization text, January 1998

Optimised polarimeter configurations for measuring the Stokes parameters of the Cosmic Microwave Background Radiation text, January 1998

The Polarbear-2 and the Simons Array Experiments journal, January 2016

Low-Temperature Detectors for CMB Imaging Arrays journal, August 2018

On-Sky Performance of the SPT-3G Frequency-Domain Multiplexed Readout journal, December 2019

Testing general relativity in cosmology journal, December 2018

Iterative map-making with two-level preconditioning for polarized cosmic microwave background data sets: A worked example for ground-based experiments journal, October 2018

Dark matter and dark energy interactions: theoretical challenges, cosmological implications and observational signatures journal, August 2016

Searching for primordial magnetic fields with CMB B -modes journal, May 2018

Recent discoveries from the cosmic microwave background: a review of recent progress journal, February 2018

Stochastic gravitational wave backgrounds journal, November 2018

Clustering fossil from primordial gravitational waves in anisotropic inflation journal, October 2015

Robust forecasts on fundamental physics from the foreground-obscured, gravitationally-lensed CMB polarization journal, March 2016

CMB-lensing beyond the Born approximation journal, September 2016

The Atacama Cosmology Telescope: two-season ACTPol spectra and parameters journal, June 2017

Exploring cosmic origins with CORE: Survey requirements and mission design journal, April 2018

Inflation physics from the cosmic microwave background and large scale structure
journal, March 2015

Neutrino physics from the cosmic microwave background and large scale structure
journal, March 2015

The POLARBEAR CMB polarization experiment
conference, July 2010

SPTpol: an instrument for CMB polarization measurements with the South Pole Telescope
conference, September 2012

Statistical properties of polarized radio sources at high frequency and their impact on cosmic microwave background polarization measurements: Properties of polarized radio sources
journal, January 2011

Non-Gaussian structure of the lensed CMB power spectra covariance matrix
journal, December 2012

Detection of $B$ -Mode Polarization at Degree Angular Scales by BICEP2
journal, June 2014

The 10 Meter South Pole Telescope
journal, May 2011

Optimised polarimeter configurations for measuring the Stokes parameters of the cosmic microwave background radiation
journal, March 1999

Measurements of E-Mode Polarization and Temperature-E-Mode Correlation in the Cosmic Microwave Background from 100 Square Degrees of Sptpol data
journal, May 2015

Radio and millimeter continuum surveys and their astrophysical implications
journal, October 2009

HEALPix: A Framework for High‐Resolution Discretization and Fast Analysis of Data Distributed on the Sphere
journal, April 2005

The Herschel -SPIRE instrument and its in-flight performance
journal, July 2010

Detection of $B$ -Mode Polarization in the Cosmic Microwave Background with Data from the South Pole Telescope
journal, September 2013

Feedhorn-coupled TES polarimeter camera modules at 150 GHz for CMB polarization measurements with SPTpol
conference, October 2012

MASTER of the Cosmic Microwave Background Anisotropy Power Spectrum: A Fast Method for Statistical Analysis of Large and Complex Cosmic Microwave Background Data Sets
journal, March 2002

A Cosmic Microwave Background Lensing mass map and its Correlation with the Cosmic Infrared Background
journal, June 2013

Cosmic Microwave Background Anisotropies
journal, September 2002

A CMB polarization primer
journal, October 1997

Matplotlib: A 2D Graphics Environment
journal, January 2007

Instrumental and analytic methods for bolometric polarimetry
journal, May 2007

Statistics of cosmic microwave background polarization
journal, June 1997

Separation of Gravitational-Wave and Cosmic-Shear Contributions to Cosmic Microwave Background Polarization
journal, June 2002

Limit on the Detectability of the Energy Scale of Inflation
journal, June 2002

Cosmological parameters from CMB and other data: A Monte Carlo approach
journal, November 2002

Efficient Computation of Cosmic Microwave Background Anisotropies in Closed Friedmann‐Robertson‐Walker Models
journal, August 2000

An improved upper limit to the CMB circular polarization at large angular scales
journal, August 2013

The Atacama Cosmology Telescope: CMB polarization at 200 < ℓ < 9000
journal, October 2014

Astrophysical and cosmological information from large-scale submillimetre surveys of extragalactic sources
journal, June 2007

ACTPol: a polarization-sensitive receiver for the Atacama Cosmology Telescope
conference, July 2010

South Pole Telescope optics
journal, January 2008

Planck 2013 results. XVI. Cosmological parameters
journal, October 2014

A MEASUREMENT OF THE COSMIC MICROWAVE BACKGROUND B -MODE POLARIZATION POWER SPECTRUM AT SUB-DEGREE SCALES WITH POLARBEAR
journal, October 2014

Evidence for Gravitational Lensing of the Cosmic Microwave Background Polarization from Cross-Correlation with the Cosmic Infrared Background
journal, April 2014

Measurement of the Cosmic Microwave Background Polarization Lensing Power Spectrum with the POLARBEAR Experiment
journal, July 2014

Unbiased estimation of an angular power spectrum
journal, November 2005

SECOND AND THIRD SEASON QUaD COSMIC MICROWAVE BACKGROUND TEMPERATURE AND POLARIZATION POWER SPECTRA
journal, February 2009

Design and characterization of 90 GHz feedhorn-coupled TES polarimeter pixels in the SPTPol camera
conference, October 2012

THE FIRST PUBLIC RELEASE OF SOUTH POLE TELESCOPE DATA: MAPS OF A 95 deg ² FIELD FROM 2008 OBSERVATIONS
journal, November 2011

An upper limit to polarized submillimetre emission in Arp 220
journal, January 2007

Signature of Gravity Waves in the Polarization of the Microwave Background
journal, March 1997

Measuring Dark Matter Power Spectrum from Cosmic Microwave Background
journal, March 1999

Improved Constraints on Cosmic Microwave Background Secondary Anisotropies from the Complete 2008 South pole Telescope data
journal, July 2011

General solution to the $E − B$ mixing problem
journal, August 2007

A Measurement of the Cosmic Microwave Background Damping tail from the 2500-Square-Degree Spt-Sz Survey
journal, November 2013

Nature of the $E - B$ decomposition of CMB polarization
journal, October 2001

Gravitational lensing effect on cosmic microwave background polarization
journal, June 1998

The Herschel-SPIRE instrument and its in-flight performance
text, January 2010

Improved constraints on cosmic microwave background secondary anisotropies from the complete 2008 South Pole Telescope data
text, January 2010

SPTpol: an instrument for CMB polarization measurements with the South Pole Telescope
text, January 2012

Planck 2013 results. XVI. Cosmological parameters
text, January 2013

Detection of B-mode Polarization in the Cosmic Microwave Background with Data from the South Pole Telescope
text, January 2013

Inflation Physics from the Cosmic Microwave Background and Large Scale Structure
text, January 2013

Neutrino Physics from the Cosmic Microwave Background and Large Scale Structure
text, January 2013

Measurements of E-Mode Polarization and Temperature-E-Mode Correlation in the Cosmic Microwave Background from 100 Square Degrees of SPTpol Data
text, January 2014

A limit on the detectability of the energy scale of inflation
text, January 2002

Separation of Gravitational-Wave and Cosmic-Shear Contributions to Cosmic Microwave Background Polarization
text, January 2002

Cosmological parameters from CMB and other data: a Monte-Carlo approach
text, January 2002

Unbiased Estimation of an Angular Power Spectrum
text, January 2004

HEALPix -- a Framework for High Resolution Discretization, and Fast Analysis of Data Distributed on the Sphere
text, January 2004

Statistics of Cosmic Microwave Background Polarization
text, January 1996

Gravitational Lensing Effect on Cosmic Microwave Background Polarization
text, January 1998

Optimised polarimeter configurations for measuring the Stokes parameters of the Cosmic Microwave Background Radiation
text, January 1998

The Polarbear-2 and the Simons Array Experiments
journal, January 2016

Low-Temperature Detectors for CMB Imaging Arrays
journal, August 2018

On-Sky Performance of the SPT-3G Frequency-Domain Multiplexed Readout
journal, December 2019

Testing general relativity in cosmology
journal, December 2018

Iterative map-making with two-level preconditioning for polarized cosmic microwave background data sets: A worked example for ground-based experiments
journal, October 2018

Dark matter and dark energy interactions: theoretical challenges, cosmological implications and observational signatures
journal, August 2016

Searching for primordial magnetic fields with CMB B -modes
journal, May 2018

Recent discoveries from the cosmic microwave background: a review of recent progress
journal, February 2018

Stochastic gravitational wave backgrounds
journal, November 2018

Clustering fossil from primordial gravitational waves in anisotropic inflation
journal, October 2015

Robust forecasts on fundamental physics from the foreground-obscured, gravitationally-lensed CMB polarization
journal, March 2016

CMB-lensing beyond the Born approximation
journal, September 2016

The Atacama Cosmology Telescope: two-season ACTPol spectra and parameters
journal, June 2017

Exploring cosmic origins with CORE: Survey requirements and mission design
journal, April 2018

Dark energy, α-attractors, and large-scale structure surveys
journal, June 2018

CMB lensing reconstruction biases in cross-correlation with large-scale structure probes
journal, October 2019

CMB lensing tomography with the DES Science Verification galaxies
journal, January 2016