A Comparison of Maps and Power Spectra Determined from South Pole Telescope and Planck Data

Hou, Z.; Aylor, K.; Benson, B. A.; Bleem, L. E.; Carlstrom, J. E.; Chang, C. L.; Cho, H-M.; Chown, R.; Crawford, T. M.; Crites, A. T.; de Haan, T.; Dobbs, M. A.; Everett, W. B.; Follin, B.; George, E. M.; Halverson, N. W.; Harrington, N. L.; Holder, G. P.; Holzapfel, W. L.; Hrubes, J. D.; Keisler, R.; Knox, L.; Lee, A. T.; Leitch, E. M.; Luong-Van, D.; Marrone, D. P.; McMahon, J. J.; Meyer, S. S.; Millea, M.; Mocanu, L. M.; Mohr, J. J.; Natoli, T.; Omori, Y.; Padin, S.; Pryke, C.; Reichardt, C. L.; Ruhl, J. E.; Sayre, J. T.; Schaffer, K. K.; Shirokoff, E.; Staniszewski, Z.; Stark, A. A.; Story, K. T.; Vanderlinde, K.; Vieira, J. D.; Williamson, R.

doi:10.3847/1538-4357/aaa3ef

Title: A Comparison of Maps and Power Spectra Determined from South Pole Telescope and Planck Data

Abstract

We study the consistency of 150 GHz data from the South Pole Telescope (SPT) and 143 GHz data from the Planck satellite over the 2540 deg2 patch of sky covered by the SPT-SZ survey. We first visually compare the maps and find that the map residuals appear consistent with noise after we account for differences in angular resolution and filtering. To make a more quantitative comparison, we calculate (1) the cross-spectrum between two independent halves of SPT 150 GHz data, (2) the cross-spectrum between two independent halves of Planck 143 GHz data, and (3) the cross-spectrum between SPT 150 GHz and Planck 143 GHz data. We find the three cross-spectra are well-fit (PTE = 0.30) by the null hypothesis in which both experiments have measured the same sky map up to a single free parameter characterizing the relative calibration between the two. As a by-product of this analysis, we improve the calibration of SPT data by nearly an order of magnitude, from 2.6% to 0.3% in power; the best-fit power calibration factor relative to the most recent published SPT calibration is 1.0174 ± 0.0033. Finally, we compare all three cross-spectra to the full-sky Planck 143 × 143 power spectrum andmore »« less

Authors:

Hou, Z. ^[1]; Aylor, K. ^[2]; Benson, B. A. ^[3]; Bleem, L. E. ^[4]; Carlstrom, J. E. ^[5]; Chang, C. L. ^[6]; Cho, H-M. ^[7]; Chown, R. ^[8];

^[1]; Crites, A. T. ^[9];

^[10]; Dobbs, M. A. ^[11]; Everett, W. B. ^[12]; Follin, B. ^[2];

^[13]; Halverson, N. W. ^[14]; Harrington, N. L. ^[15];

^[16]; Holzapfel, W. L. ^[15]; Hrubes, J. D. ^[17] more »

Univ. of Chicago, IL (United States). Kavli Inst. for Cosmological Physics; Univ. of Chicago, IL (United States). Dept. of Astronomy and Astrophysics
Univ. of California, Davis, CA (United States). Dept. of Physics
Univ. of Chicago, IL (United States). Kavli Inst. for Cosmological Physics; 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; Argonne National Lab. (ANL), Argonne, IL (United States). High Energy Physics Division
Univ. of Chicago, IL (United States). Kavli Inst. for Cosmological Physics; Univ. of Chicago, IL (United States). Dept. of Astronomy and Astrophysics; Argonne National Lab. (ANL), Argonne, IL (United States). High Energy Physics Division; Univ. of Chicago, IL (United States). Dept. of Physics; Univ. of Chicago, IL (United States). Enrico Fermi Inst.
Univ. of Chicago, IL (United States). Kavli Inst. for Cosmological Physics; Univ. of Chicago, IL (United States). Dept. of Astronomy and Astrophysics; Argonne National Lab. (ANL), Argonne, IL (United States). High Energy Physics Division
SLAC National Accelerator Lab., Menlo Park, CA (United States)
McGill Univ., Montreal, QC (Canada). Dept of Physics and McGill Space Inst.
Univ. of Chicago, IL (United States). Kavli Inst. for Cosmological Physics; 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 and McGill Space Inst.; Univ. of California, Berkeley, CA (United States). Dept. of Physics
McGill Univ., Montreal, QC (Canada). Dept of Physics and McGill Space Inst.; Canadian Inst. for Advanced Research, Toronto, ON (Canada). CIFAR Program in Cosmology and Gravity
Univ. of Colorado, Boulder, CO (United States). Center for Astrophysics and Space Astronomy, Dept. of Astrophysical and Planetary Sciences
Univ. of California, Berkeley, CA (United States). Dept. of Physics; European Southern Observatory, Garching (Germany)
Univ. of Colorado, Boulder, CO (United States). Center for Astrophysics and Space Astronomy, Dept. of Astrophysical and Planetary Sciences; Univ. of Colorado, Boulder, CO (United States). Dept. of Physics
Univ. of California, Berkeley, CA (United States). Dept. of Physics
McGill Univ., Montreal, QC (Canada). Dept of Physics and McGill Space Inst.; Canadian Inst. for Advanced Research, Toronto, ON (Canada). CIFAR Program in Cosmology and Gravity; Univ. of Illinois, Urbana, IL (United States). Astronomy Dept.; Univ. of Illinois, Urbana, IL (United States). Dept. of Physics
Univ. of Chicago, IL (United States)
Univ. of Chicago, IL (United States). Kavli Inst. for Cosmological Physics; Univ. of Chicago, IL (United States). Dept. of Physics; Stanford Univ., CA (United States). Kavli Inst. for Particle Astrophysics and Cosmology
Univ. of California, Berkeley, CA (United States). Dept. of Physics; Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States). Physics Division
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; 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.
Ludwig Maximilian Univ., Munich (Germany). Faculty of Physics
Univ. of Chicago, IL (United States). Kavli Inst. for Cosmological Physics; Univ. of Chicago, IL (United States). Dept. of Physics; Univ. of Toronto, ON (Canada). Dunlap Inst. for Astronomy & Astrophysics
Univ. of Minnesota, Minneapolis, MN (United States). Dept. of Physics
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, Dept. of Physics
Univ. of Colorado, Boulder, CO (United States). Center for Astrophysics and Space Astronomy, Dept. of Astrophysical and Planetary Sciences; Case Western Reserve Univ., Cleveland, OH (United States). Center for Education and Research in Cosmology and Astrophysics, Dept. of Physics
Univ. of Chicago, IL (United States). Kavli Inst. for Cosmological Physics; Univ. of Chicago, IL (United States). Enrico Fermi Inst.; School of the Art Institute of Chicago, Chicago, IL (United States). Liberal Arts Dept.
Univ. of Chicago, IL (United States). Kavli Inst. for Cosmological Physics; Univ. of Chicago, IL (United States). Dept. of Astronomy and Astrophysics; Univ. of California, Berkeley, CA (United States). Dept. of Physics
Case Western Reserve Univ., Cleveland, OH (United States). Center for Education and Research in Cosmology and Astrophysics, Dept. of Physics; California Inst. of Technology (CalTech), Pasadena, CA (United States). Jet Propulsion Lab.
Harvard-Smithsonian Center for Astrophysics, Cambridge, MA (United States)
Univ. of Chicago, IL (United States). Kavli Inst. for Cosmological Physics; Univ. of Chicago, IL (United States). Dept. of Physics; Stanford Univ., CA (United States). Kavli Inst. for Particle Astrophysics and Cosmology; Stanford Univ., CA (United States). Dept. of Physics
Univ. of Toronto, ON (Canada). Dunlap Inst. for Astronomy & Astrophysics; Univ. of Toronto, ON (Canada). Dept. of Astronomy & Astrophysics
Univ. of Illinois, Urbana, IL (United States). Dept. of Astronomy; Univ. of Illinois, Urbana, IL (United States). Dept. of Physics

Publication Date:: 2018-01-17

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

Sponsoring Org.:: National Science Foundation (NSF); Gordon and Betty Moore Foundation (GBMF); Engineering Research Council of Canada; Australian Research Council (ARC); USDOE Office of Science (SC), High Energy Physics (HEP); Gordon and Betty Moore Foundation; USDOE Office of Science (SC), Basic Energy Sciences (BES)

OSTI Identifier:: 1419974

Alternate Identifier(s):: OSTI ID: 1354868; OSTI ID: 1426763

Report Number(s):: FERMILAB-PUB-17-094-AE; arXiv:1704.00884
Journal ID: ISSN 1538-4357; TRN: US1801423

Grant/Contract Number:: AC02-76SF00515; AC02-06CH11357; AC02-07CH11359; PLR-1248097; PHY-1125897; GBMF 947

Resource Type:: Accepted Manuscript

Journal Name:: The Astrophysical Journal (Online)

Additional Journal Information:: Journal Name: The Astrophysical Journal (Online); Journal Volume: 853; 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; methods: data analysis

Citation Formats


                    Hou, Z., Aylor, K., Benson, B. A., Bleem, L. E., Carlstrom, J. E., Chang, C. L., Cho, H-M., Chown, R., Crawford, T. M., Crites, A. T., de Haan, T., Dobbs, M. A., Everett, W. B., Follin, B., George, E. M., Halverson, N. W., Harrington, N. L., Holder, G. P., Holzapfel, W. L., Hrubes, J. D., Keisler, R., Knox, L., Lee, A. T., Leitch, E. M., Luong-Van, D., Marrone, D. P., McMahon, J. J., Meyer, S. S., Millea, M., Mocanu, L. M., Mohr, J. J., Natoli, T., Omori, Y., Padin, S., Pryke, C., Reichardt, C. L., Ruhl, J. E., Sayre, J. T., Schaffer, K. K., Shirokoff, E., Staniszewski, Z., Stark, A. A., Story, K. T., Vanderlinde, K., Vieira, J. D., and Williamson, R.. A Comparison of Maps and Power Spectra Determined from South Pole Telescope and Planck Data.  United States: N. p., 2018. 
Web.  doi:10.3847/1538-4357/aaa3ef.

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                    Hou, Z., Aylor, K., Benson, B. A., Bleem, L. E., Carlstrom, J. E., Chang, C. L., Cho, H-M., Chown, R., Crawford, T. M., Crites, A. T., de Haan, T., Dobbs, M. A., Everett, W. B., Follin, B., George, E. M., Halverson, N. W., Harrington, N. L., Holder, G. P., Holzapfel, W. L., Hrubes, J. D., Keisler, R., Knox, L., Lee, A. T., Leitch, E. M., Luong-Van, D., Marrone, D. P., McMahon, J. J., Meyer, S. S., Millea, M., Mocanu, L. M., Mohr, J. J., Natoli, T., Omori, Y., Padin, S., Pryke, C., Reichardt, C. L., Ruhl, J. E., Sayre, J. T., Schaffer, K. K., Shirokoff, E., Staniszewski, Z., Stark, A. A., Story, K. T., Vanderlinde, K., Vieira, J. D., & Williamson, R.. A Comparison of Maps and Power Spectra Determined from South Pole Telescope and Planck Data.  United States.  https://doi.org/10.3847/1538-4357/aaa3ef

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                    Hou, Z., Aylor, K., Benson, B. A., Bleem, L. E., Carlstrom, J. E., Chang, C. L., Cho, H-M., Chown, R., Crawford, T. M., Crites, A. T., de Haan, T., Dobbs, M. A., Everett, W. B., Follin, B., George, E. M., Halverson, N. W., Harrington, N. L., Holder, G. P., Holzapfel, W. L., Hrubes, J. D., Keisler, R., Knox, L., Lee, A. T., Leitch, E. M., Luong-Van, D., Marrone, D. P., McMahon, J. J., Meyer, S. S., Millea, M., Mocanu, L. M., Mohr, J. J., Natoli, T., Omori, Y., Padin, S., Pryke, C., Reichardt, C. L., Ruhl, J. E., Sayre, J. T., Schaffer, K. K., Shirokoff, E., Staniszewski, Z., Stark, A. A., Story, K. T., Vanderlinde, K., Vieira, J. D., and Williamson, R.. Wed .  
"A Comparison of Maps and Power Spectra Determined from South Pole Telescope and Planck Data".  United States.  https://doi.org/10.3847/1538-4357/aaa3ef.  https://www.osti.gov/servlets/purl/1419974.

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@article{osti_1419974,

  title        = {A Comparison of Maps and Power Spectra Determined from South Pole Telescope and Planck Data},

  author       = {Hou, Z. and Aylor, K. and Benson, B. A. and Bleem, L. E. and Carlstrom, J. E. and Chang, C. L. and Cho, H-M. and Chown, R. and Crawford, T. M. and Crites, A. T. and de Haan, T. and Dobbs, M. A. and Everett, W. B. and Follin, B. and George, E. M. and Halverson, N. W. and Harrington, N. L. and Holder, G. P. and Holzapfel, W. L. and Hrubes, J. D. and Keisler, R. and Knox, L. and Lee, A. T. and Leitch, E. M. and Luong-Van, D. and Marrone, D. P. and McMahon, J. J. and Meyer, S. S. and Millea, M. and Mocanu, L. M. and Mohr, J. J. and Natoli, T. and Omori, Y. and Padin, S. and Pryke, C. and Reichardt, C. L. and Ruhl, J. E. and Sayre, J. T. and Schaffer, K. K. and Shirokoff, E. and Staniszewski, Z. and Stark, A. A. and Story, K. T. and Vanderlinde, K. and Vieira, J. D. and Williamson, R.},

  abstractNote = {We study the consistency of 150 GHz data from the South Pole Telescope (SPT) and 143 GHz data from the Planck satellite over the 2540 deg2 patch of sky covered by the SPT-SZ survey. We first visually compare the maps and find that the map residuals appear consistent with noise after we account for differences in angular resolution and filtering. To make a more quantitative comparison, we calculate (1) the cross-spectrum between two independent halves of SPT 150 GHz data, (2) the cross-spectrum between two independent halves of Planck 143 GHz data, and (3) the cross-spectrum between SPT 150 GHz and Planck 143 GHz data. We find the three cross-spectra are well-fit (PTE = 0.30) by the null hypothesis in which both experiments have measured the same sky map up to a single free parameter characterizing the relative calibration between the two. As a by-product of this analysis, we improve the calibration of SPT data by nearly an order of magnitude, from 2.6% to 0.3% in power; the best-fit power calibration factor relative to the most recent published SPT calibration is 1.0174 ± 0.0033. Finally, we compare all three cross-spectra to the full-sky Planck 143 × 143 power spectrum and find a hint (~1.5σ) for differences in the power spectrum of the SPT-SZ footprint and the full-sky power spectrum, which we model and fit as a power law in the spectrum. The best-fit value of this tilt is consistent between the three cross-spectra in the SPT-SZ footprint, implying that the source of this tilt—assuming it is real—is a sample variance fluctuation in the SPT-SZ region relative to the full sky. Despite the precision of our tests, we find no evidence for systematic errors in either data set. The consistency of cosmological parameters derived from these datasets is discussed in a companion paper.},

  doi          = {10.3847/1538-4357/aaa3ef},

  journal      = {The Astrophysical Journal (Online)},

  number       = 1,

  volume       = 853,

  place        = {United States},

  year         = {2018},

  month        = {1}

}

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FiG 1: The celestial southern hemisphere of CMB data from Planck HFI 143 GHz data. The black curve outlines the SPT-SZ survey coverage. The image is oriented such that the line of 0^h right ascension extends from the center to the top of the hemisphere, and right ascension increases counter-clockwise.

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DOI: 10.1051/0004-6361/201525813

Planck 2015 results : X. Diffuse component separation: Foreground maps
journal, September 2016

Adam, R.; Ade, P. A. R.; Aghanim, N.
Astronomy & Astrophysics, Vol. 594
DOI: 10.1051/0004-6361/201525967

Planck 2015 results : XVI. Isotropy and statistics of the CMB
journal, September 2016

Ade, P. A. R.; Aghanim, N.; Akrami, Y.
Astronomy & Astrophysics, Vol. 594
DOI: 10.1051/0004-6361/201526681

Planck 2015 results : XXVI. The Second
journal, September 2016

Ade, P. A. R.; Aghanim, N.; Argüeso, F.
Astronomy & Astrophysics, Vol. 594
DOI: 10.1051/0004-6361/201526914

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

Shaw, Laurie D.; Nagai, Daisuke; Bhattacharya, Suman
arXiv
DOI: 10.48550/arxiv.1006.1945

A Measurement of the Damping Tail of the Cosmic Microwave Background Power Spectrum with the South Pole Telescope
text, January 2011

Keisler, R.; Reichardt, C. L.; Aird, K. A.
arXiv
DOI: 10.48550/arxiv.1105.3182

Deconstructing the kinetic SZ Power Spectrum
text, January 2011

Shaw, Laurie D.; Rudd, Douglas H.; Nagai, Daisuke
arXiv
DOI: 10.48550/arxiv.1109.0553

Constraints on Cosmology from the Cosmic Microwave Background Power Spectrum of the 2500 ${\rm deg}^2$ SPT-SZ Survey
text, January 2012

Hou, Z.; Reichardt, C. L.; Story, K. T.
arXiv
DOI: 10.48550/arxiv.1212.6267

A hybrid model for the evolution of galaxies and Active Galactic Nuclei in the infrared
text, January 2013

Cai, Zhen-Yi; Lapi, Andrea; Xia, Jun-Qing
arXiv
DOI: 10.48550/arxiv.1303.2335

Planck 2013 results. I. Overview of products and scientific results
text, January 2013

Collaboration, Planck; Ade, P. A. R.; Aghanim, N.
arXiv
DOI: 10.48550/arxiv.1303.5062

Planck 2013 results. VII. HFI time response and beams
text, January 2013

Collaboration, Planck; Ade, P. A. R.; Aghanim, N.
arXiv
DOI: 10.48550/arxiv.1303.5068

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

Collaboration, Planck; Ade, P. A. R.; Aghanim, N.
arXiv
DOI: 10.48550/arxiv.1303.5076

Planck 2015 results. XIII. Cosmological parameters
text, January 2015

Collaboration, Planck; Ade, P. A. R.; Aghanim, N.
arXiv
DOI: 10.48550/arxiv.1502.01589

Planck 2015 results. XI. CMB power spectra, likelihoods, and robustness of parameters
text, January 2015

Collaboration, Planck; Aghanim, N.; Arnaud, M.
arXiv
DOI: 10.48550/arxiv.1507.02704

Quantifying discordance in the 2015 Planck CMB spectrum
text, January 2015

Addison, G. E.; Huang, Y.; Watts, D. J.
arXiv
DOI: 10.48550/arxiv.1511.00055

A 2.4% Determination of the Local Value of the Hubble Constant
text, January 2016

Riess, Adam G.; Macri, Lucas M.; Hoffmann, Samantha L.
arXiv
DOI: 10.48550/arxiv.1604.01424

A Comparison of Cosmological Parameters Determined from CMB Temperature Power Spectra from the South Pole Telescope and the Planck Satellite
text, January 2017

Aylor, K.; Hou, Z.; Knox, L.
arXiv
DOI: 10.48550/arxiv.1706.10286

Fast estimation of polarization power spectra using correlation functions
text, January 2003

Chon, Gayoung; Challinor, Anthony; Prunet, Simon
arXiv
DOI: 10.48550/arxiv.astro-ph/0303414

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

Gorski, K. M.; Hivon, E.; Banday, A. J.
arXiv
DOI: 10.48550/arxiv.astro-ph/0409513

Predictions for high-frequency radio surveys of extragalactic sources
text, January 2004

De Zotti, Gianfranco; Ricci, Roberto; Mesa, Dino
arXiv
DOI: 10.48550/arxiv.astro-ph/0410709

Cosmic Microwave Background Anisotropy Window Functions Revisited
text, January 1999

Knox, Lloyd
arXiv
DOI: 10.48550/arxiv.astro-ph/9902046

Works referencing / citing this record:

Maps of the Southern Millimeter-wave Sky from Combined 2500 deg ² SPT-SZ and Planck Temperature Data
journal, November 2018

Chown, R.; Omori, Y.; Aylor, K.
The Astrophysical Journal Supplement Series, Vol. 239, Issue 1
DOI: 10.3847/1538-4365/aae694

Measurements of the Cross-spectra of the Cosmic Infrared and Microwave Backgrounds from 95 to 1200 GHz
journal, August 2019

Viero, M. P.; Reichardt, C. L.; Benson, B. A.
The Astrophysical Journal, Vol. 881, Issue 2
DOI: 10.3847/1538-4357/ab2da0

Sounds Discordant: Classical Distance Ladder and ΛCDM-based Determinations of the Cosmological Sound Horizon
journal, March 2019

Aylor, Kevin; Joy, Mackenzie; Knox, Lloyd
The Astrophysical Journal, Vol. 874, Issue 1
DOI: 10.3847/1538-4357/ab0898

Assessing Consistency between WMAP 9 Year and Planck 2015 Temperature Power Spectra
journal, December 2018

Huang, Y.; Addison, G. E.; Weiland, J. L.
The Astrophysical Journal, Vol. 869, Issue 1
DOI: 10.3847/1538-4357/aaeb1f

Analytic Calculation of Covariance between Cosmological Parameters from Correlated Data Sets, with an Application to SPTpol
journal, December 2019

Kable, Joshua A.; Addison, Graeme E.; Bennett, Charles L.
The Astrophysical Journal, Vol. 888, Issue 1
DOI: 10.3847/1538-4357/ab54cc

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We present three maps of the millimeter-wave sky created by combining data from the South Pole Telescope (SPT) and the Planck satellite. We use data from the SPT-SZ survey, a survey of 2540 deg2 of the the sky with arcminute resolution in three bands centered at 95, 150, and 220 GHz, and the full-mission Planck temperature data in the 100, 143, and 217 GHz bands. A linear combination of the SPT-SZ and Planck data is computed in spherical harmonic space, with weights derived from the noise of both instruments. This weighting scheme results in Planck data providing most of themore »« less
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Title: A Comparison of Maps and Power Spectra Determined from South Pole Telescope and Planck Data

Abstract

Citation Formats

Figures / Tables:

Planck 2013 results. VII. HFI time response and beams journal, October 2014

Planck 2015 results : VIII. High Frequency Instrument data processing: Calibration and maps journal, September 2016

Planck 2015 results : VII. High Frequency Instrument data processing: Time-ordered information and beams journal, September 2016

Planck 2015 results : XII. Full focal plane simulations journal, September 2016

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

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

Fast Cosmic Microwave Background Analyses via Correlation Functions journal, February 2001

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

NINE-YEAR WILKINSON MICROWAVE ANISOTROPY PROBE ( WMAP ) OBSERVATIONS: FINAL MAPS AND RESULTS journal, September 2013

Predictions for high-frequency radio surveys of extragalactic sources journal, February 2005

The Atacama Cosmology Telescope: cross correlation with Planck maps journal, July 2014

Planck 2015 results : XI. CMB power spectra, likelihoods, and robustness of parameters journal, September 2016

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

Planck 2015 results : XIII. Cosmological parameters journal, September 2016

Planck 2015 results : XXIV. Cosmology from Sunyaev-Zeldovich cluster counts journal, September 2016

Planck 2013 results. I. Overview of products and scientific results journal, October 2014

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

A Comparison of Cosmological Parameters Determined from CMB Temperature Power Spectra from the South Pole Telescope and the Planck Satellite journal, November 2017

Planck intermediate results : LI. Features in the cosmic microwave background temperature power spectrum and shifts in cosmological parameters journal, November 2017

Herschel observations and a model for IRAS 08572+3915: a candidate for the most luminous infrared galaxy in the local (z < 0.2) Universe journal, October 2013

Fast estimation of polarization power spectra using correlation functions journal, May 2004

QUANTIFYING DISCORDANCE IN THE 2015 PLANCK CMB SPECTRUM journal, February 2016

Evidence for Massive Neutrinos from Cosmic Microwave Background and Lensing Observations journal, February 2014

A Hybrid Model for the Evolution of Galaxies and Active Galactic Nuclei in the Infrared journal, April 2013

Cosmological parameters from pre-planck cosmic microwave background measurements journal, May 2013

A Measurement of Secondary Cosmic Microwave Background Anisotropies from the 2500 Square-Degree Spt-Sz Survey journal, January 2015

CONSTRAINTS ON COSMOLOGY FROM THE COSMIC MICROWAVE BACKGROUND POWER SPECTRUM OF THE 2500 deg 2 SPT-SZ SURVEY journal, January 2014

A Measurement of the Damping tail of the Cosmic Microwave Background Power Spectrum with the South pole Telescope journal, November 2011

Cosmic microwave background anisotropy window functions revisited journal, October 1999

Lensed CMB simulation and parameter estimation journal, April 2005

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

A 3% SOLUTION: DETERMINATION OF THE HUBBLE CONSTANT WITH THE HUBBLE SPACE TELESCOPE AND WIDE FIELD CAMERA 3 journal, March 2011

A 2.4% Determination of the Local Value of the Hubble Constant journal, July 2016

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

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

Deconstructing the Kinetic sz Power Spectrum journal, August 2012

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

Neutrinos Help Reconcile Planck Measurements with the Local Universe journal, February 2014

Planck intermediate results: XVII. Emission of dust in the diffuse interstellar medium from the far-infrared to microwave frequencies⋆ journal, June 2014

Planck 2015 results : VI. LFI mapmaking journal, September 2016

Planck 2015 results : X. Diffuse component separation: Foreground maps journal, September 2016

Planck 2015 results : XVI. Isotropy and statistics of the CMB journal, September 2016

Planck 2015 results : XXVI. The Second journal, September 2016

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

A Measurement of the Damping Tail of the Cosmic Microwave Background Power Spectrum with the South Pole Telescope text, January 2011

Deconstructing the kinetic SZ Power Spectrum text, January 2011

Constraints on Cosmology from the Cosmic Microwave Background Power Spectrum of the 2500 ${\rm deg}^2$ SPT-SZ Survey text, January 2012

A hybrid model for the evolution of galaxies and Active Galactic Nuclei in the infrared text, January 2013

Planck 2013 results. I. Overview of products and scientific results text, January 2013

Planck 2013 results. VII. HFI time response and beams text, January 2013

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

Planck 2015 results. XIII. Cosmological parameters text, January 2015

Planck 2015 results. XI. CMB power spectra, likelihoods, and robustness of parameters text, January 2015

Quantifying discordance in the 2015 Planck CMB spectrum text, January 2015

A 2.4% Determination of the Local Value of the Hubble Constant text, January 2016

A Comparison of Cosmological Parameters Determined from CMB Temperature Power Spectra from the South Pole Telescope and the Planck Satellite text, January 2017

Fast estimation of polarization power spectra using correlation functions text, January 2003

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

Predictions for high-frequency radio surveys of extragalactic sources text, January 2004

Cosmic Microwave Background Anisotropy Window Functions Revisited text, January 1999

Maps of the Southern Millimeter-wave Sky from Combined 2500 deg 2 SPT-SZ and Planck Temperature Data journal, November 2018

Measurements of the Cross-spectra of the Cosmic Infrared and Microwave Backgrounds from 95 to 1200 GHz journal, August 2019

Sounds Discordant: Classical Distance Ladder and ΛCDM-based Determinations of the Cosmological Sound Horizon journal, March 2019

Assessing Consistency between WMAP 9 Year and Planck 2015 Temperature Power Spectra journal, December 2018

Analytic Calculation of Covariance between Cosmological Parameters from Correlated Data Sets, with an Application to SPTpol journal, December 2019

Planck 2013 results. VII. HFI time response and beams
journal, October 2014

Planck 2015 results : VIII. High Frequency Instrument data processing: Calibration and maps
journal, September 2016

Planck 2015 results : VII. High Frequency Instrument data processing: Time-ordered information and beams
journal, September 2016

Planck 2015 results : XII. Full focal plane simulations
journal, September 2016

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

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

Fast Cosmic Microwave Background Analyses via Correlation Functions
journal, February 2001

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

NINE-YEAR WILKINSON MICROWAVE ANISOTROPY PROBE ( WMAP ) OBSERVATIONS: FINAL MAPS AND RESULTS
journal, September 2013

Predictions for high-frequency radio surveys of extragalactic sources
journal, February 2005

The Atacama Cosmology Telescope: cross correlation with Planck maps
journal, July 2014

Planck 2015 results : XI. CMB power spectra, likelihoods, and robustness of parameters
journal, September 2016

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

Planck 2015 results : XIII. Cosmological parameters
journal, September 2016

Planck 2015 results : XXIV. Cosmology from Sunyaev-Zeldovich cluster counts
journal, September 2016

Planck 2013 results. I. Overview of products and scientific results
journal, October 2014

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

A Comparison of Cosmological Parameters Determined from CMB Temperature Power Spectra from the South Pole Telescope and the Planck Satellite
journal, November 2017

Planck intermediate results : LI. Features in the cosmic microwave background temperature power spectrum and shifts in cosmological parameters
journal, November 2017

Herschel observations and a model for IRAS 08572+3915: a candidate for the most luminous infrared galaxy in the local (z < 0.2) Universe
journal, October 2013

Fast estimation of polarization power spectra using correlation functions
journal, May 2004

QUANTIFYING DISCORDANCE IN THE 2015 PLANCK CMB SPECTRUM
journal, February 2016

Evidence for Massive Neutrinos from Cosmic Microwave Background and Lensing Observations
journal, February 2014

A Hybrid Model for the Evolution of Galaxies and Active Galactic Nuclei in the Infrared
journal, April 2013

Cosmological parameters from pre-planck cosmic microwave background measurements
journal, May 2013

A Measurement of Secondary Cosmic Microwave Background Anisotropies from the 2500 Square-Degree Spt-Sz Survey
journal, January 2015

CONSTRAINTS ON COSMOLOGY FROM THE COSMIC MICROWAVE BACKGROUND POWER SPECTRUM OF THE 2500 deg ² SPT-SZ SURVEY
journal, January 2014

A Measurement of the Damping tail of the Cosmic Microwave Background Power Spectrum with the South pole Telescope
journal, November 2011

Cosmic microwave background anisotropy window functions revisited
journal, October 1999

Lensed CMB simulation and parameter estimation
journal, April 2005

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

A 3% SOLUTION: DETERMINATION OF THE HUBBLE CONSTANT WITH THE HUBBLE SPACE TELESCOPE AND WIDE FIELD CAMERA 3
journal, March 2011

A 2.4% Determination of the Local Value of the Hubble Constant
journal, July 2016

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

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

Deconstructing the Kinetic sz Power Spectrum
journal, August 2012

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

Neutrinos Help Reconcile Planck Measurements with the Local Universe
journal, February 2014

Planck intermediate results: XVII. Emission of dust in the diffuse interstellar medium from the far-infrared to microwave frequencies⋆
journal, June 2014

Planck 2015 results : VI. LFI mapmaking
journal, September 2016

Planck 2015 results : X. Diffuse component separation: Foreground maps
journal, September 2016

Planck 2015 results : XVI. Isotropy and statistics of the CMB
journal, September 2016

Planck 2015 results : XXVI. The Second
journal, September 2016

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

A Measurement of the Damping Tail of the Cosmic Microwave Background Power Spectrum with the South Pole Telescope
text, January 2011

Deconstructing the kinetic SZ Power Spectrum
text, January 2011

Constraints on Cosmology from the Cosmic Microwave Background Power Spectrum of the 2500 ${\rm deg}^2$ SPT-SZ Survey
text, January 2012

A hybrid model for the evolution of galaxies and Active Galactic Nuclei in the infrared
text, January 2013

Planck 2013 results. I. Overview of products and scientific results
text, January 2013

Planck 2013 results. VII. HFI time response and beams
text, January 2013

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

Planck 2015 results. XIII. Cosmological parameters
text, January 2015

Planck 2015 results. XI. CMB power spectra, likelihoods, and robustness of parameters
text, January 2015

Quantifying discordance in the 2015 Planck CMB spectrum
text, January 2015

A 2.4% Determination of the Local Value of the Hubble Constant
text, January 2016

A Comparison of Cosmological Parameters Determined from CMB Temperature Power Spectra from the South Pole Telescope and the Planck Satellite
text, January 2017

Fast estimation of polarization power spectra using correlation functions
text, January 2003

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

Predictions for high-frequency radio surveys of extragalactic sources
text, January 2004

Cosmic Microwave Background Anisotropy Window Functions Revisited
text, January 1999

Maps of the Southern Millimeter-wave Sky from Combined 2500 deg ² SPT-SZ and Planck Temperature Data
journal, November 2018

Measurements of the Cross-spectra of the Cosmic Infrared and Microwave Backgrounds from 95 to 1200 GHz
journal, August 2019

Sounds Discordant: Classical Distance Ladder and ΛCDM-based Determinations of the Cosmological Sound Horizon
journal, March 2019

Assessing Consistency between WMAP 9 Year and Planck 2015 Temperature Power Spectra
journal, December 2018

Analytic Calculation of Covariance between Cosmological Parameters from Correlated Data Sets, with an Application to SPTpol
journal, December 2019