Journal article

Detection of CMB-Cluster Lensing using Polarization Data from SPTpol

S Raghunathan, S Patil, E Baxter, BA Benson, LE Bleem, TM Crawford, GP Holder, T McClintock, CL Reichardt, TN Varga, N Whitehorn, PAR Ade, S Allam, AJ Anderson, JE Austermann, S Avila, JS Avva, D Bacon, JA Beall, AN Bender Show all

PHYSICAL REVIEW LETTERS | AMER PHYSICAL SOC | Published : 2019

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Awarded by NSF


Awarded by Australian Research Council


Awarded by U.S. Department of Energy


Awarded by National Science Foundation


Awarded by NSF Physics Frontier Center


Awarded by Gordon and Betty Moore Foundation


Awarded by Office of Science of the U.S. Department of Energy


Awarded by MINECO


Awarded by European Research Council


Awarded by Australian Research Council Centre of Excellence for All-sky Astrophysics (CAASTRO)


Awarded by Brazilian Instituto Nacional de Ciencia e Tecnologia (INCT) e-Universe (CNPq)


Awarded by Fermi Research Alliance, LLC


Funding Acknowledgements

The authors thank Andrew Ludwig, Nickolas McColl, Siavash Yasini, and the three anonymous reviewers for their valuable feedback on the manuscript. S. R. acknowledges partial support from the Laby Foundation. S. P. acknowledges support from Melbourne International Engagement Award (MIPP) and Laby Travel Bursary. The UCLA authors acknowledge support from NSF Grants No. AST-1716965 and No. CSSI-1835865. The Melbourne group acknowledges support from the Australian Research Council's Discovery Projects scheme (Grant No. DP150103208). The work of L. B. was supported under the U.S. Department of Energy Contract No. DE-AC02-06CH11357. We acknowledge the use of CAMB [29] software. This work was performed in the context of the South Pole Telescope scientific program. S. P. T. is supported by the National Science Foundation through Grant No. PLR-1248097. Partial support is also provided by the NSF Physics Frontier Center Grant No. PHY-1125897 to the Kavli Institute of Cosmological Physics at the University of Chicago, the Kavli Foundation, and the Gordon and Betty Moore Foundation Grant No. GBMF 947. This research used resources of the National Energy Research Scientific Computing Center (NERSC), a DOE Office of Science User Facility supported by the Office of Science of the U.S. Department of Energy under Contract No. DE-AC02-05CH11231. Funding for the DES Projects has been provided by the U.S. Department of Energy, the U.S. National Science Foundation, the Ministry of Science and Education of Spain, the Science and Technology Facilities Council of the United Kingdom, the Higher Education Funding Council for England, the National Center for Supercomputing Applications at the University of Illinois at Urbana-Champaign, the Kavli Institute of Cosmological Physics at the University of Chicago, the Center for Cosmology and Astro-Particle Physics at the Ohio State University, the Mitchell Institute for Fundamental Physics and Astronomy at Texas A&M University, Financiadora de Estudos e Projetos, Fundacao Carlos Chagas Filho de Amparo a Pesquisa do Estado do Rio de Janeiro, Conselho Nacional de Desenvolvimento Cientifico e Tecnologico and the Ministerio da Ciencia, Tecnologia e Inovacao, the Deutsche Forschungsgemeinschaft and the Collaborating Institutions in the Dark Energy Survey. The Collaborating Institutions are Argonne National Laboratory, the University of California at Santa Cruz, the University of Cambridge, Centro de Investigaciones Energeticas, Medioambientales y Tecnologicas-Madrid, the University of Chicago, University College London, the DES-Brazil Consortium, the University of Edinburgh, the Eidgenossische Technische Hochschule (ETH) Zurich, Fermi National Accelerator Laboratory, the University of Illinois at Urbana-Champaign, the Institut de Ciencies de l'Espai (IEEC/CSIC), the Institut de Fisica d'Altes Energies, Lawrence Berkeley National Laboratory, the Ludwig-Maximilians Universitat Munchen and the associated Excellence Cluster Universe, the University of Michigan, the National Optical Astronomy Observatory, the University of Nottingham, The Ohio State University, the University of Pennsylvania, the University of Portsmouth, SLAC National Accelerator Laboratory, Stanford University, the University of Sussex, Texas A&M University, and the OzDES Membership Consortium.This work is based in part on observations at Cerro Tololo Inter-American Observatory, National Optical Astronomy Observatory, which is operated by the Association of Universities for Research in Astronomy (AURA) under a cooperative agreement with the National Science Foundation. The DES data management system is supported by the National Science Foundation under Grants No. AST-1138766 and No. AST-1536171. The DES participants from Spanish institutions are partially supported by MINECO under Grants No. AYA2015-71825, No. ESP2015-66861, No. FPA2015-68048, No. SEV-2016-0588, No. SEV-2016-0597, and No. MDM-20150509, some of which include ERDF funds from the European Union. I. F. A. E. is partially funded by the CERCA program of the Generalitat de Catalunya. Research leading to these results has received funding from the European Research Council under the European Union's Seventh Framework Program (No. FP7/2007-2013) including ERC Grants No. 240672, No. 291329, and No. 306478. We acknowledge support from the Australian Research Council Centre of Excellence for All-sky Astrophysics (CAASTRO), through Project No. CE110001020, and the Brazilian Instituto Nacional de Ciencia e Tecnologia (INCT) e-Universe (CNPq Grant No. 465376/2014-2). This manuscript has been coauthored by employees of the Fermi Research Alliance, LLC under Contract No. DE-AC02-07CH11359 with the U.S. Department of Energy, Office of Science, Office of High Energy Physics. The United States Government retains and the publisher, by accepting the article for publication, acknowledges that the United States Government retains a nonexclusive, paid-up, irrevocable, world-wide license to publish or reproduce the published form of this manuscript, or allow others to do so, for United States Government purposes.