A measurement of the cosmic microwave background gravitational lensing potential from 100 square degrees of SPTpol data

Story, K. T.; Hanson, D.; 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.; Harrington, N.; Henning, J. W.; Hilton, G. C.; Holder, G. P.; Holzapfel, W. L.; Hoover, S.; Hou, Z.; Hrubes, J. D.; Huang, N.; Hubmayr, J.; Irwin, K. D.; Keisler, R.; Knox, L.; Lee, A. T.; Leitch, E. M.; Li, D.; Liang, C.; Luong-Van, D.; McMahon, J. J.; Mehl, J.; Meyer, S. S.; Mocanu, L.; Montroy, T. E.; 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.; Smecher, G.; Stark, A. A.; Tucker, C.; Vanderlinde, K.; Vieira, J. D.; Wang, G.; Whitehorn, N.; Yefremenko, V.; Zahn, O.

doi:10.1088/0004-637X/810/1/50

Title: A measurement of the cosmic microwave background gravitational lensing potential from 100 square degrees of SPTpol data

Abstract

Here, we present a measurement of the cosmic microwave background (CMB) gravitational lensing potential using data from the first two seasons of observations with SPTpol, the polarization-sensitive receiver currently installed on the South Pole Telescope. The observations used in this work cover 100 deg² of sky with arcminute resolution at 150 GHz. Using a quadratic estimator, we make maps of the CMB lensing potential from combinations of CMB temperature and polarization maps. We combine these lensing potential maps to form a minimum-variance (MV) map. The lensing potential is measured with a signal-to-noise ratio of greater than one for angular multipoles between $$100\lt L\lt 250$$. This is the highest signal-to-noise mass map made from the CMB to date and will be powerful in cross-correlation with other tracers of large-scale structure. We calculate the power spectrum of the lensing potential for each estimator, and we report the value of the MV power spectrum between $$100\lt L\lt 2000$$ as our primary result. We constrain the ratio of the spectrum to a fiducial ΛCDM model to be AMV = 0.92 ± 0.14 (Stat.) ± 0.08 (Sys.). Restricting ourselves to polarized data only, we find A_POL = 0.92 ± 0.24 (Stat.) ± 0.11 (Sys.). This measurement rejects the hypothesis of no lensing at $$5.9\sigma $$ using polarization data alone, and at $$14\sigma $$ using both temperature and polarization data.

Authors:

Story, K. T. ^[1]; Hanson, D. ^[2]; Ade, P. A. R. ^[3]; Aird, K. A. ^[1]; Austermann, J. E. ^[4]; Beall, J. A. ^[5]; Bender, A. N. ^[6]; Benson, B. A. ^[7]; Bleem, L. E. ^[8]; Carlstrom, J. E. ^[8]; Chang, C. L. ^[8]; Chiang, H. C. ^[9]; Cho, H. -M. ^[10]; Citron, R. ^[1]; Crawford, T. M. ^[1]; Crites, A. T. ^[8]; de Haan, T. ^[11]; Dobbs, M. A. ^[12]; Everett, W. ^[4]; Gallicchio, J. ^[1] more »

Univ. of Chicago, Chicago, IL (United States)
McGill Univ., Montreal, QC (Canada)
Cardiff Univ., Cardiff (United Kingdom)
Univ. of Colorado, Boulder, CO (United States)
NIST Quantum Devices Group, Boulder, CO (United States)
McGill Univ., Montreal, QC (Canada); Argonne National Lab. (ANL), Argonne, IL (United States)
Univ. of Chicago, Chicago, IL (United States); Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States)
Univ. of Chicago, Chicago, IL (United States); Argonne National Lab. (ANL), Argonne, IL (United States)
Univ. of KwaZulu-Natal, Durban (South Africa)
SLAC National Accelerator Lab., Menlo Park, CA (United States)
Univ. of California, Berkeley, CA (United States)
McGill Univ., Montreal, QC (Canada); Canadian Institute for Advanced Research, Toronto, ON (Canada)
Univ. of Chicago, Chicago, IL (United States); Univ. of Colorado, Boulder, CO (United States)
SLAC National Accelerator Lab., Menlo Park, CA (United States); Stanford Univ., Stanford, CA (United States)
Stanford Univ., Stanford, CA (United States)
Univ. of California, Davis, CA (United States)
Univ. of California, Berkeley, CA (United States); Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States)
NIST Quantum Devices Group, Boulder, CO (United States); SLAC National Accelerator Lab., Menlo Park, CA (United States)
Univ. of Michigan, Ann Arbor, MI (United States)
Case Western Reserve Univ., Cleveland, OH (United States)
Argonne National Lab. (ANL), Argonne, IL (United States)
Univ. of Chicago, Chicago, IL (United States); California Inst. of Technology (CalTech), Pasadena, CA (United States)
Univ. of Minnesota, Minneapolis, MN (United States)
Univ. of California, Berkeley, CA (United States); Univ. of Melbourne (Australia)
Univ. of Chicago, Chicago, IL (United States); School of the Art Institute of Chicago, Chicago, IL (United States)
McGill Univ., Montreal, QC (Canada); Three-Speed Logic, Inc., Vancouver, BC (Canada)
Harvard-Smithsonian Center for Astrophysics, Cambridge, MA (United States)
Univ. of Toronto, Toronto, ON (Canada)
Univ. of Illinois at Urbana-Champaign, Urbana, IL (United States)

Publication Date:: Fri Aug 28 00:00:00 EDT 2015

Research Org.:: SLAC National Accelerator Lab., Menlo Park, CA (United States)

Sponsoring Org.:: USDOE

OSTI Identifier:: 1326855

Report Number(s):: SLAC-PUB-16712
Journal ID: ISSN 1538-4357

Grant/Contract Number:: AC02-76SF00515

Resource Type:: Accepted Manuscript

Journal Name:: The Astrophysical Journal (Online)

Additional Journal Information:: Journal Name: The Astrophysical Journal (Online); Journal Volume: 810; Journal Issue: 1; 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; large-scale structure of universe

Citation Formats


                    Story, K. T., Hanson, D., 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., Harrington, N., Henning, J. W., Hilton, G. C., Holder, G. P., Holzapfel, W. L., Hoover, S., Hou, Z., Hrubes, J. D., Huang, N., Hubmayr, J., Irwin, K. D., Keisler, R., Knox, L., Lee, A. T., Leitch, E. M., Li, D., Liang, C., Luong-Van, D., McMahon, J. J., Mehl, J., Meyer, S. S., Mocanu, L., Montroy, T. E., 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., Smecher, G., Stark, A. A., Tucker, C., Vanderlinde, K., Vieira, J. D., Wang, G., Whitehorn, N., Yefremenko, V., and Zahn, O. A measurement of the cosmic microwave background gravitational lensing potential from 100 square degrees of SPTpol data.  United States: N. p., 2015. 
Web.  doi:10.1088/0004-637X/810/1/50.

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                    Story, K. T., Hanson, D., 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., Harrington, N., Henning, J. W., Hilton, G. C., Holder, G. P., Holzapfel, W. L., Hoover, S., Hou, Z., Hrubes, J. D., Huang, N., Hubmayr, J., Irwin, K. D., Keisler, R., Knox, L., Lee, A. T., Leitch, E. M., Li, D., Liang, C., Luong-Van, D., McMahon, J. J., Mehl, J., Meyer, S. S., Mocanu, L., Montroy, T. E., 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., Smecher, G., Stark, A. A., Tucker, C., Vanderlinde, K., Vieira, J. D., Wang, G., Whitehorn, N., Yefremenko, V., & Zahn, O. A measurement of the cosmic microwave background gravitational lensing potential from 100 square degrees of SPTpol data.  United States.  https://doi.org/10.1088/0004-637X/810/1/50

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                    Story, K. T., Hanson, D., 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., Harrington, N., Henning, J. W., Hilton, G. C., Holder, G. P., Holzapfel, W. L., Hoover, S., Hou, Z., Hrubes, J. D., Huang, N., Hubmayr, J., Irwin, K. D., Keisler, R., Knox, L., Lee, A. T., Leitch, E. M., Li, D., Liang, C., Luong-Van, D., McMahon, J. J., Mehl, J., Meyer, S. S., Mocanu, L., Montroy, T. E., 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., Smecher, G., Stark, A. A., Tucker, C., Vanderlinde, K., Vieira, J. D., Wang, G., Whitehorn, N., Yefremenko, V., and Zahn, O. Fri .  
"A measurement of the cosmic microwave background gravitational lensing potential from 100 square degrees of SPTpol data".  United States.  https://doi.org/10.1088/0004-637X/810/1/50.  https://www.osti.gov/servlets/purl/1326855.

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@article{osti_1326855,

  title        = {A measurement of the cosmic microwave background gravitational lensing potential from 100 square degrees of SPTpol data},

  author       = {Story, K. T. and Hanson, D. 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 Harrington, N. and Henning, J. W. and Hilton, G. C. and Holder, G. P. and Holzapfel, W. L. and Hoover, S. and Hou, Z. and Hrubes, J. D. and Huang, N. and Hubmayr, J. and Irwin, K. D. and Keisler, R. and Knox, L. and Lee, A. T. and Leitch, E. M. and Li, D. and Liang, C. and Luong-Van, D. and McMahon, J. J. and Mehl, J. and Meyer, S. S. and Mocanu, L. and Montroy, T. E. 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 Smecher, G. and Stark, A. A. and Tucker, C. and Vanderlinde, K. and Vieira, J. D. and Wang, G. and Whitehorn, N. and Yefremenko, V. and Zahn, O.},

  abstractNote = {Here, we present a measurement of the cosmic microwave background (CMB) gravitational lensing potential using data from the first two seasons of observations with SPTpol, the polarization-sensitive receiver currently installed on the South Pole Telescope. The observations used in this work cover 100 deg2 of sky with arcminute resolution at 150 GHz. Using a quadratic estimator, we make maps of the CMB lensing potential from combinations of CMB temperature and polarization maps. We combine these lensing potential maps to form a minimum-variance (MV) map. The lensing potential is measured with a signal-to-noise ratio of greater than one for angular multipoles between $100\lt L\lt 250$. This is the highest signal-to-noise mass map made from the CMB to date and will be powerful in cross-correlation with other tracers of large-scale structure. We calculate the power spectrum of the lensing potential for each estimator, and we report the value of the MV power spectrum between $100\lt L\lt 2000$ as our primary result. We constrain the ratio of the spectrum to a fiducial ΛCDM model to be AMV = 0.92 ± 0.14 (Stat.) ± 0.08 (Sys.). Restricting ourselves to polarized data only, we find APOL = 0.92 ± 0.24 (Stat.) ± 0.11 (Sys.). This measurement rejects the hypothesis of no lensing at $5.9\sigma $ using polarization data alone, and at $14\sigma $ using both temperature and polarization data.},

  doi          = {10.1088/0004-637X/810/1/50},

  journal      = {The Astrophysical Journal (Online)},

  number       = 1,

  volume       = 810,

  place        = {United States},

  year         = {Fri Aug 28 00:00:00 EDT 2015},

  month        = {Fri Aug 28 00:00:00 EDT 2015}

}

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Title: A measurement of the cosmic microwave background gravitational lensing potential from 100 square degrees of SPTpol data

Abstract

Citation Formats

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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

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

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

Impact of Cluster Physics on the Sunyaev-Zel'Dovich Power Spectrum journal, November 2010

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Full-sky lensing reconstruction of gradient and curl modes from CMB maps text, January 2011

Bias-Hardened CMB Lensing text, January 2012

The Atacama Cosmology Telescope: Temperature and Gravitational Lensing Power Spectrum Measurements from Three Seasons of Data text, January 2013

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CMB Lensing Power Spectrum Biases from Galaxies and Clusters using High-angular Resolution Temperature Maps text, January 2013

Precision Epoch of Reionization studies with next-generation CMB experiments text, January 2014

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

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Gravitational Lensing Effect on Cosmic Microwave Background Anisotropies: a Power Spectrum Approach text, January 1995

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

Planck 2015 results : XXIII. The thermal Sunyaev-Zeldovich effect-cosmic infrared background correlation journal, September 2016

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

CMB-lensing beyond the Born approximation journal, September 2016

CMB delensing beyond the B modes journal, December 2017

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CMB Polarization B -mode Delensing with SPTpol and Herschel journal, August 2017

A 2500 deg 2 CMB Lensing Map from Combined South Pole Telescope and Planck Data journal, November 2017

Measurements of the Temperature and E-mode Polarization of the CMB from 500 Square Degrees of SPTpol Data journal, January 2018

Constraints on Cosmological Parameters from the Angular Power Spectrum of a Combined 2500 deg 2 SPT-SZ and Planck Gravitational Lensing Map journal, June 2018

Evidence for the Cross-correlation between Cosmic Microwave Background Polarization Lensing from Polarbear and Cosmic Shear from Subaru Hyper Suprime-Cam journal, September 2019

A Measurement of the Cosmic Microwave Background Lensing Potential and Power Spectrum from 500 deg 2 of SPTpol Temperature and Polarization Data journal, October 2019

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

CMB lensing constraints on dark energy and modified gravity scenarios
journal, November 2009

Precision epoch of reionization studies with next-generation CMB experiments
journal, August 2014

The 10 Meter South Pole Telescope
journal, May 2011

Gravitational lensing of fluctuations in the microwave background radiation
journal, July 1989

Cosmic shear of the microwave background: The curl diagnostic
journal, June 2005

The Atacama Cosmology Telescope: temperature and gravitational lensing power spectrum measurements from three seasons of data
journal, April 2014

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

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journal, September 2013

NINE-YEAR WILKINSON MICROWAVE ANISOTROPY PROBE ( WMAP ) OBSERVATIONS: COSMOLOGICAL PARAMETER RESULTS
journal, September 2013

Correlation of CMB with large-scale structure. II. Weak lensing
journal, August 2008

Mapping the Dark Matter through the Cosmic Microwave Background Damping Tail
journal, August 2001

Mass Reconstruction with Cosmic Microwave Background Polarization
journal, August 2002

A CMB polarization primer
journal, October 1997

Matplotlib: A 2D Graphics Environment
journal, January 2007

Lensing reconstruction with CMB temperature and polarization
journal, June 2003

Massive neutrinos and cosmology
journal, July 2006

Lensed CMB simulation and parameter estimation
journal, April 2005

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

Weak gravitational lensing of the CMB
journal, June 2006

The shape of the CMB lensing bispectrum
journal, March 2011

EXTRAGALACTIC MILLIMETER-WAVE POINT-SOURCE CATALOG, NUMBER COUNTS AND STATISTICS FROM 771 deg ² OF THE SPT-SZ SURVEY
journal, November 2013

Bias-hardened CMB lensing
journal, February 2013

Full-sky lensing reconstruction of gradient and curl modes from CMB maps
journal, January 2012

Extragalactic foreground contamination in temperature-based CMB lens reconstruction
journal, March 2014

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

Gravitational Lensing Effect on Cosmic Microwave Background Anisotropies: A Power Spectrum Approach
journal, May 1996

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

Impact of Cluster Physics on the Sunyaev-Zel'Dovich Power Spectrum
journal, November 2010

Detection of gravitational lensing in the cosmic microwave background
journal, August 2007

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

Cmb Lensing Power Spectrum Biases from Galaxies and Clusters Using High-Angular Resolution Temperature maps
journal, April 2014

A Measurement of Gravitational Lensing of the Microwave Background Using South pole Telescope data
journal, August 2012

Galaxy Clusters Selected with the Sunyaev-Zel'Dovich Effect from 2008 South pole Telescope Observations
journal, September 2010

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

Correlation of CMB with large-scale structure. II. Weak lensing
text, January 2008

Galaxy Clusters Selected with the Sunyaev-Zel'dovich Effect from 2008 South Pole Telescope Observations
text, January 2010

Impact of Cluster Physics on the Sunyaev-Zel'dovich Power Spectrum
text, January 2010

Full-sky lensing reconstruction of gradient and curl modes from CMB maps
text, January 2011

Bias-Hardened CMB Lensing
text, January 2012

The Atacama Cosmology Telescope: Temperature and Gravitational Lensing Power Spectrum Measurements from Three Seasons of Data
text, January 2013

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

CMB Lensing Power Spectrum Biases from Galaxies and Clusters using High-angular Resolution Temperature Maps
text, January 2013

Precision Epoch of Reionization studies with next-generation CMB experiments
text, January 2014

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

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

Cosmic Shear of the Microwave Background: The Curl Diagnostic
text, January 2005

Weak Gravitational Lensing of the CMB
text, January 2006

Gravitational Lensing Effect on Cosmic Microwave Background Anisotropies: a Power Spectrum Approach
text, January 1995

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

Planck 2015 results : XXIII. The thermal Sunyaev-Zeldovich effect-cosmic infrared background correlation
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Recent discoveries from the cosmic microwave background: a review of recent progress
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CMB-lensing beyond the Born approximation
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CMB delensing beyond the B modes
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Real space lensing reconstruction using cosmic microwave background polarization
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The Simons Observatory: science goals and forecasts
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CMB lensing reconstruction biases in cross-correlation with large-scale structure probes
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CMB lensing tomography with the DES Science Verification galaxies
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Constraining gravity at the largest scales through CMB lensing and galaxy velocities
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Cross-correlation of gravitational lensing from DES Science Verification data with SPT and Planck lensing
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Exploring suppressed long-distance correlations as the cause of suppressed large-angle correlations
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Probing gravitational lensing of the CMB with SDSS-IV quasars
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Distortions in the surface of last scattering
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Optimal filtering for CMB lensing reconstruction
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Year two instrument status of the SPT-3G cosmic microwave background receiver
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Bicep2/ KECK ARRAY VIII: MEASUREMENT OF GRAVITATIONAL LENSING FROM LARGE-SCALE B -MODE POLARIZATION
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Planck Lensing and Cosmic Infrared Background Cross-correlation with Fermi -LAT: Tracing Dark Matter Signals in the Gamma-Ray Background
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CMB Polarization B -mode Delensing with SPTpol and Herschel
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A 2500 deg ² CMB Lensing Map from Combined South Pole Telescope and Planck Data
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Measurements of the Temperature and E-mode Polarization of the CMB from 500 Square Degrees of SPTpol Data
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Constraints on Cosmological Parameters from the Angular Power Spectrum of a Combined 2500 deg ² SPT-SZ and Planck Gravitational Lensing Map
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Evidence for the Cross-correlation between Cosmic Microwave Background Polarization Lensing from Polarbear and Cosmic Shear from Subaru Hyper Suprime-Cam
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A Measurement of the Cosmic Microwave Background Lensing Potential and Power Spectrum from 500 deg ² of SPTpol Temperature and Polarization Data
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Cross-correlation of CMB Polarization Lensing with High- z Submillimeter Herschel -ATLAS Galaxies
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Constraints on Cosmological Parameters from the 500 deg ² SPTPOL Lensing Power Spectrum
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Planck 2015 results : XIII. Cosmological parameters
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