AuthorMarrone, D P
AffiliationUniv Arizona, Steward Observ
Keywordsgravitational lensing: weak
large-scale structure of Universe
MetadataShow full item record
PublisherOXFORD UNIV PRESS
CitationJ Prat, E Baxter, T Shin, C Sánchez, C Chang, B Jain, R Miquel, A Alarcon, D Bacon, G M Bernstein, R Cawthon, T M Crawford, C Davis, J De Vicente, S Dodelson, T F Eifler, O Friedrich, M Gatti, D Gruen, W G Hartley, G P Holder, B Hoyle, M Jarvis, E Krause, N MacCrann, B Mawdsley, A Nicola, Y Omori, A Pujol, M M Rau, C L Reichardt, S Samuroff, E Sheldon, M A Troxel, P Vielzeuf, J Zuntz, T M C Abbott, F B Abdalla, J Annis, S Avila, K Aylor, B A Benson, E Bertin, L E Bleem, D Brooks, D L Burke, J E Carlstrom, M Carrasco Kind, J Carretero, C L Chang, H-M Cho, R Chown, A T Crites, C E Cunha, L N da Costa, S Desai, H T Diehl, J P Dietrich, M A Dobbs, P Doel, W B Everett, A E Evrard, B Flaugher, P Fosalba, J García-Bellido, E Gaztanaga, E M George, D W Gerdes, T Giannantonio, R A Gruendl, J Gschwend, G Gutierrez, T de Haan, N W Halverson, N L Harrington, W L Holzapfel, K Honscheid, Z Hou, J D Hrubes, D J James, T Jeltema, L Knox, R Kron, K Kuehn, N Kuropatkin, O Lahav, A T Lee, E M Leitch, M Lima, D Luong-Van, M A G Maia, A Manzotti, D P Marrone, J L Marshall, J J McMahon, P Melchior, F Menanteau, S S Meyer, C J Miller, L M Mocanu, J J Mohr, T Natoli, S Padin, A A Plazas, C Pryke, A K Romer, A Roodman, J E Ruhl, E S Rykoff, E Sanchez, J T Sayre, V Scarpine, K K Schaffer, S Serrano, I Sevilla-Noarbe, E Shirokoff, G Simard, M Smith, M Soares-Santos, F Sobreira, Z Staniszewski, A A Stark, K T Story, E Suchyta, M E C Swanson, G Tarle, D Thomas, K Vanderlinde, J D Vieira, V Vikram, A R Walker, J Weller, R Williamson, O Zahn, (The DES and SPT Collaborations), Cosmological lensing ratios with DES Y1, SPT, and Planck, Monthly Notices of the Royal Astronomical Society, Volume 487, Issue 1, July 2019, Pages 1363–1379, https://doi.org/10.1093/mnras/stz1309
RightsCopyright © 2019 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society This article is published and distributed under the terms of the Oxford University Press, Standard Journals Publication Model (https://academic.oup.com/journals/pages/open_access/funder_policies/chorus/standard_publication_model)
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AbstractCorrelations between tracers of the matter density field and gravitational lensing are sensitive to the evolution of the matter power spectrum and the expansion rate across cosmic time. Appropriately defined ratios of such correlation functions, on the other hand, depend only on the angular diameter distances to the tracer objects and to the gravitational lensing source planes. Because of their simple cosmological dependence, such ratios can exploit available signal-to-noise ratio down to small angular scales, even where directly modelling the correlation functions is difficult. We present a measurement of lensing ratios using galaxy position and lensing data from the Dark Energy Survey, and CMB lensing data from the South Pole Telescope and Planck, obtaining the highest precision lensing ratio measurements to date. Relative to the concordance Lambda CDM model, we find a best-fitting lensing ratio amplitude of A = 1.1 +/- 0.1. We use the ratio measurements to generate cosmological constraints, focusing on the curvature parameter. We demonstrate that photometrically selected galaxies can be used to measure lensing ratios, and argue that future lensing ratio measurements with data from a combination of LSST and Stage-4 CMB experiments can be used to place interesting cosmological constraints, even after considering the systematic uncertainties associated with photometric redshift and galaxy shear estimation.
VersionFinal published version
SponsorsU.S. Department of Energy; U.S. National Science Foundation; Ministry of Science and Education of Spain; Science and Technology Facilities Council of the United Kingdom; Higher Education Funding Council for England; National Center for Supercomputing Applications at the University of Illinois at Urbana-Champaign; Kavli Institute of Cosmological Physics at the University of Chicago; Center for Cosmology and Astro-Particle Physics at the Ohio State University; Mitchell Institute for Fundamental Physics and Astronomy at Texas AM University; Financiadora de Estudos e Projetos; Conselho Nacional de Desenvolvimento Cientifico e Tecnologico; Ministerio da Ciencia, Tecnologia e Inovacao; Deutsche Forschungsgemeinschaft; Argonne National Laboratory; University of California at Santa Cruz; University of Cambridge; University College London; DES-Brazil Consortium; University of Edinburgh; Eidgenossische Technische Hochschule (ETH) Zurich; Fermi National Accelerator Laboratory; University of Illinois at Urbana-Champaign; Institut de Ciencies de l'Espai (IEEC/CSIC); Institut de Fisica d'Altes Energies; Lawrence Berkeley National Laboratory; Ludwig-Maximilians Universitat Munchen; University of Michigan; National Optical Astronomy Observatory; University of Nottingham; Ohio State University; University of Pennsylvania; University of Portsmouth; SLAC National Accelerator Laboratory; Stanford University; University of Sussex; Texas AM University; OzDES Membership Consortium; National Science Foundation [AST-1138766, AST-1536171]; MINECO [AYA2015-71825, ESP2015-66861, FPA2015-68048, SEV-2016-0588, SEV-2016-0597, MDM-2015-0509]; ERDF funds from the European Union; CERCA program of the Generalitat de Catalunya; European Research Council under the European Union; ERC [240672, 291329, 306478]; Australian Research Council Centre of Excellence for All-sky Astrophysics (CAASTRO) [CE110001020]; Brazilian Instituto Nacional de Ciencia e Tecnologia (INCT) e-Universe (CNPq) [465376/2014-2]; U.S. Department of Energy, Office of Science, Office of High Energy Physics [DE-AC02-07CH11359]; Fundacao Carlos Chagas Filho de Amparo a Pesquisa do Estado do Rio de Janeiro