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Title: A measurement of gravitational lensing of the cosmic microwave background by galaxy clusters using data from the south pole telescope

Journal Article · · Astrophysical Journal
 [1]; ; ;  [2]; ; ; ; ;  [3];  [4];  [5]; ;  [6];  [7]; ; ;  [8];  [9];  [10];  [11] more »; « less
  1. Center for Particle Cosmology, Department of Physics and Astronomy, University of Pennsylvania, Philadelphia, PA 19104 (United States)
  2. Kavli Institute for Cosmological Physics, University of Chicago, Chicago, IL 60637 (United States)
  3. Department of Astronomy and Astrophysics, University of Chicago, Chicago, IL 60637 (United States)
  4. University of Chicago, Chicago, IL 60637 (United States)
  5. Kavli Institute for Particle Astrophysics and Cosmology, Stanford University, 452 Lomita Mall, Stanford, CA 94305 (United States)
  6. Harvard-Smithsonian Center for Astrophysics, Cambridge, MA 02138 (United States)
  7. Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology, 77 Massachusetts Avenue, Cambridge, MA 02139 (United States)
  8. Department of Physics, Ludwig-Maximilians-Universität, D-81679 München (Germany)
  9. Department of Physics and Astronomy, University of Missouri, 5110 Rockhill Road, Kansas City, MO 64110 (United States)
  10. NIST Quantum Devices Group, Boulder, CO 80305 (United States)
  11. Departamento de Astronomia y Astrosifica, Pontificia Universidad Catolica (Chile)

Clusters of galaxies are expected to gravitationally lens the cosmic microwave background (CMB) and thereby generate a distinct signal in the CMB on arcminute scales. Measurements of this effect can be used to constrain the masses of galaxy clusters with CMB data alone. Here we present a measurement of lensing of the CMB by galaxy clusters using data from the South Pole Telescope (SPT). We develop a maximum likelihood approach to extract the CMB cluster lensing signal and validate the method on mock data. We quantify the effects on our analysis of several potential sources of systematic error and find that they generally act to reduce the best-fit cluster mass. It is estimated that this bias to lower cluster mass is roughly 0.85σ in units of the statistical error bar, although this estimate should be viewed as an upper limit. We apply our maximum likelihood technique to 513 clusters selected via their Sunyaev–Zeldovich (SZ) signatures in SPT data, and rule out the null hypothesis of no lensing at 3.1σ. The lensing-derived mass estimate for the full cluster sample is consistent with that inferred from the SZ flux: M{sub 200,lens}=0.83{sub −0.37}{sup +0.38} M{sub 200,SZ} (68% C.L., statistical error only).

OSTI ID:
22883004
Journal Information:
Astrophysical Journal, Vol. 806, Issue 2; Other Information: Country of input: International Atomic Energy Agency (IAEA); Since 2009, the country of publication for this journal is the UK.; ISSN 0004-637X
Country of Publication:
United Kingdom
Language:
English

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Planck 2015 results : XIII. Cosmological parameters journal September 2016
Recent discoveries from the cosmic microwave background: a review of recent progress journal February 2018
Measuring galaxy cluster masses with CMB lensing using a Maximum Likelihood estimator: statistical and systematic error budgets for future experiments journal August 2017
Real space lensing reconstruction using cosmic microwave background polarization journal January 2018
Exploring cosmic origins with CORE: Cluster science journal April 2018
Exploring cosmic origins with CORE: Mitigation of systematic effects journal April 2018
Neutrino mass and dark energy constraints from redshift-space distortions journal May 2019
Constraining the rotational kinematic Sunyaev-Zel'dovich effect in massive galaxy clusters journal June 2019
Bias to CMB lensing from lensed foregrounds journal December 2019
Looking through the same lens: Shear calibration for LSST, Euclid, and WFIRST with stage 4 CMB lensing journal June 2017
Maximum a posteriori CMB lensing reconstruction journal September 2017
Bias to CMB lensing reconstruction from temperature anisotropies due to large-scale galaxy motions journal January 2018
Mitigating foreground biases in CMB lensing reconstruction using cleaned gradients journal July 2018
Detection of CMB-Cluster Lensing using Polarization Data from SPTpol journal October 2019
Imaging cosmic polarization rotation journal October 2016
The Simons Observatory: Science goals and forecasts text January 2019
Cosmological Constraints from Galaxy Clusters in the 2500 Square-Degree Spt-Sz Survey journal November 2016
Mass Calibration of Optically Selected DES Clusters Using a Measurement of CMB-cluster Lensing with SPTpol Data journal February 2019
The Halo Mass of Optically Luminous Quasars at z ≈ 1–2 Measured via Gravitational Deflection of the Cosmic Microwave Background journal March 2019
Suppressing the Thermal SZ-induced Variance in CMB-cluster Lensing Estimators journal December 2019
Pairwise Transverse Velocity Measurement with the Rees–Sciama Effect journal March 2019
Planck 2015 results : VI. LFI mapmaking journal September 2016
The Simons Observatory: science goals and forecasts journal February 2019
Planck 2015 results : XVI. Isotropy and statistics of the CMB journal September 2016
Planck 2015 results : XXVI. The Second journal September 2016
Planck 2015 results : XXIV. Cosmology from Sunyaev-Zeldovich cluster counts journal September 2016
Exploring Cosmic Origins with CORE: Cluster Science text January 2017
Bias to CMB Lensing Reconstruction from Temperature Anisotropies due to Large-Scale Galaxy Motions text January 2017
Real space lensing reconstruction using cosmic microwave background polarization text January 2017
Mitigating Foreground Biases in CMB Lensing Reconstruction Using Cleaned Gradients text January 2018
The Simons Observatory: Science goals and forecasts text January 2018
Mass Calibration of Optically Selected DES clusters using a Measurement of CMB-Cluster Lensing with SPTpol Data text January 2018
Pairwise Transverse Velocity Measurement with the Rees-Sciama Effect text January 2018
The halo mass of optically-luminous quasars at z=1-2 measured via gravitational deflection of the cosmic microwave background text January 2019