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Dark Energy Survey Year 3 Results: Three-point shear correlations and mass aperture moments

Secco, L. F. and Jarvis, M. and Jain, B. and Chang, C. and Gatti, M. and Frieman, J. and Adhikari, S. and Alarcon, A. and Amon, A. and Bechtol, K. and Becker, M. R. and Bernstein, G. M. and Blazek, J. and Campos, A. and Carnero Rosell, A. and Carrasco Kind, M. and Choi, A. and Cordero, J. and DeRose, J. and Dodelson, S. and Doux, C. and Drlica-Wagner, A. and Everett, S. and Giannini, G. and Gruen, D. and Gruendl, R. A. and Harrison, I. and Hartley, W. G. and Herner, K. and Krause, E. and MacCrann, N. and McCullough, J. and Myles, J. and Navarro-Alsina, A. and Prat, J. and Rollins, R. P. and Samuroff, S. and Sánchez, C. and Sevilla-Noarbe, I. and Sheldon, E. and Troxel, M. A. and Zeurcher, D. and Aguena, M. and Andrade-Oliveira, F. and Annis, J. and Bacon, D. and Bertin, E. and Bocquet, S. and Brooks, D. and Burke, D. L. and Carretero, J. and Castander, F. J. and Crocce, M. and da Costa, L. N. and Pereira, M. E. S. and De Vicente, J. and Diehl, H. T. and Doel, P. and Eckert, K. and Ferrero, I. and Flaugher, B. and Friedel, D. and García-Bellido, J. and Gutierrez, G. and Hinton, S. R. and Hollowood, D. L. and Honscheid, K. and Huterer, D. and Kuehn, K. and Kuropatkin, N. and Maia, M. A. G. and Marshall, J. L. and Menanteau, F. and Miquel, R. and Mohr, J. J. and Morgan, R. and Muir, J. and Paz-Chinchón, F. and Pieres, A. and Plazas Malagón, A. A. and Rodriguez-Monroy, M. and Roodman, A. and Sanchez, E. and Serrano, S. and Suchyta, E. and Swanson, M. E. C. and Tarle, G. and Thomas, D. and To, C. and Weller, J. (2022) Dark Energy Survey Year 3 Results: Three-point shear correlations and mass aperture moments. Physical Review D, 105 (10). Art. No. 103537. ISSN 2470-0010. doi:10.1103/physrevd.105.103537. https://resolver.caltech.edu/CaltechAUTHORS:20220608-849415000

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Abstract

We present high signal-to-noise measurements of three-point shear correlations and the third moment of the mass aperture statistic using the first 3 years of data from the Dark Energy Survey. We additionally obtain the first measurements of the configuration and scale dependence of the four three-point shear correlations which carry cosmological information. With the third-order mass aperture statistic, we present tomographic measurements over angular scales of 4 to 60 arcminutes with a combined statistical significance of 15.0 σ . Using the tomographic information and measuring also the second-order mass aperture, we additionally obtain a skewness parameter and its redshift evolution. We find that the amplitudes and scale-dependence of these shear 3pt functions are in qualitative agreement with measurements in a mock galaxy catalog based on N-body simulations, indicating promise for including them in future cosmological analyses. We validate our measurements by showing that B-modes, parity-violating contributions and PSF modeling uncertainties are negligible, and determine that the measured signals are likely to be of astrophysical and gravitational origin.


Item Type:Article
Related URLs:
URLURL TypeDescription
https://doi.org/10.1103/PhysRevD.105.103537DOIArticle
https://arxiv.org/abs/2201.05227arXivDiscussion Paper
ORCID:
AuthorORCID
Jarvis, M.0000-0001-7039-9078
Frieman, J.0000-0003-4079-3263
Bechtol, K.0000-0001-8156-0429
Carnero Rosell, A.0000-0003-3044-5150
Carrasco Kind, M.0000-0002-4802-3194
Choi, A.0000-0002-5636-233X
Gruen, D.0000-0003-3270-7644
Prat, J.0000-0002-5933-5150
Sevilla-Noarbe, I.0000-0002-1831-1953
Annis, J.0000-0002-0609-3987
Bertin, E.0000-0002-3602-3664
Bocquet, S.0000-0002-4900-805X
Brooks, D.0000-0002-8458-5047
Carretero, J.0000-0002-3130-0204
De Vicente, J.0000-0001-8318-6813
Ferrero, I.0000-0002-1295-1132
Flaugher, B.0000-0002-2367-5049
García-Bellido, J.0000-0002-9370-8360
Gutierrez, G.0000-0003-0825-0517
Honscheid, K.0000-0002-6550-2023
Kuehn, K.0000-0003-0120-0808
Kuropatkin, N.0000-0003-2511-0946
Menanteau, F.0000-0002-1372-2534
Miquel, R.0000-0002-6610-4836
Paz-Chinchón, F.0000-0003-1339-2683
Roodman, A.0000-0001-5326-3486
Suchyta, E.0000-0002-7047-9358
Tarle, G.0000-0003-1704-0781
To, C.0000-0001-7836-2261
Weller, J.0000-0002-8282-2010
Additional Information:© 2022 American Physical Society. (Received 24 January 2022; accepted 26 April 2022; published 31 May 2022) We would like to thank Lucas Porth for comments and Ryuichi Takahashi and collaborators for making the T17 simulations utilized in this work publicly available. This work was completed in part with resources provided by the University of Chicago Research Computing Center. M. J. is supported in part by National Science Foundation Grant No. 1907610. B. J. is supported in part by the U.S. Department of Energy Grant No. DE-SC0007901. C. C. is supported by DOE grant DE-SC0021949. 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, Fundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de Janeiro, Conselho Nacional de Desenvolvimento Científico e Tecnológico and the Ministério da Ciência, Tecnologia e Inovação, 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 Energéticas, Medioambientales y Tecnológicas-Madrid, the University of Chicago, University College London, the DES-Brazil Consortium, the University of Edinburgh, the Eidgenössische Technische Hochschule (ETH) Zürich, Fermi National Accelerator Laboratory, the University of Illinois at Urbana-Champaign, the Institut de Ciències de l’Espai (IEEC/CSIC), the Institut de Física d’Altes Energies, Lawrence Berkeley National Laboratory, the Ludwig-Maximilians Universität München 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. 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 MICINN under Grants No. ESP2017-89838, No. PGC2018-094773, No. PGC2018-102021, No. SEV-2016-0588, No. SEV-2016-0597, and No. MDM-2015-0509, some of which include ERDF funds from the European Union. IFAE 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 (FP7/2007-2013) including ERC Grants agreements No. 240672, No. 291329, and No. 306478. We acknowledge support from the Brazilian Instituto Nacional de Ciência e Tecnologia (INCT) do e-Universo (CNPq Grant No. 465376/2014-2). We acknowledge support from the Australian Research Council Centre of Excellence for All-sky Astrophysics (CAASTRO), through Project No. CE110001020. This manuscript has been authored by 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. 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. This work made use of Matplotlib [78] and NASA’s Astrophysics Data System Bibliographic Services (ADS).
Funders:
Funding AgencyGrant Number
NSFAST-1907610
Department of Energy (DOE)DE-SC0007901
Department of Energy (DOE)DE-SC0021949
NSFAST-1138766
NSFAST-1536171
Science and Technology Facilities Council (STFC)UNSPECIFIED
Higher Education Funding Council for EnglandUNSPECIFIED
University of Illinois at Urbana-ChampaignUNSPECIFIED
University of ChicagoUNSPECIFIED
Ohio State UniversityUNSPECIFIED
Texas A&M UniversityUNSPECIFIED
Financiadora de Estudos e Projetos (FINEP)UNSPECIFIED
Fundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de Janeiro (FAPERJ)UNSPECIFIED
Conselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq)465376/2014-2
Ministério da Ciência, Tecnologia e InovaçãoUNSPECIFIED
Deutsche Forschungsgemeinschaft (DFG)UNSPECIFIED
Argonne National LaboratoryUNSPECIFIED
University of California, Santa CruzUNSPECIFIED
University of CambridgeUNSPECIFIED
Centro de Investigaciones Energéticas, Medioambientales y TecnológicasUNSPECIFIED
University College LondonUNSPECIFIED
University of EdinburghUNSPECIFIED
ETH ZurichUNSPECIFIED
FermilabUNSPECIFIED
Institut de Física d’Altes EnergiesUNSPECIFIED
Lawrence Berkeley National LaboratoryUNSPECIFIED
Ludwig-Maximilians-Universität MünchenUNSPECIFIED
University of MichiganUNSPECIFIED
University of NottinghamUNSPECIFIED
University of PennsylvaniaUNSPECIFIED
University of PortsmouthUNSPECIFIED
SLAC National Accelerator LaboratoryUNSPECIFIED
Stanford UniversityUNSPECIFIED
University of SussexUNSPECIFIED
Ministerio de Ciencia e Innovación (MICINN)ESP2017-89838
Ministerio de Ciencia e Innovación (MICINN)PGC2018-094773
Ministerio de Ciencia e Innovación (MICINN)PGC2018-102021
Ministerio de Ciencia e Innovación (MICINN)SEV-2016-0588
Ministerio de Ciencia e Innovación (MICINN)SEV-2016-0597
Ministerio de Ciencia e Innovación (MICINN)MDM-2015-0509
European Regional Development FundUNSPECIFIED
Generalitat de CatalunyaUNSPECIFIED
European Research Council (ERC)240672
European Research Council (ERC)291329
European Research Council (ERC)306478
Instituto Nacional de Ciência e Tecnologia de Fármacos e MedicamentosUNSPECIFIED
Australian Research CouncilCE110001020
National Optical Astronomy Observatory (NOAO)UNSPECIFIED
Institut de Ciències de l’EspaiUNSPECIFIED
National Optical Astronomy ObservatoryUNSPECIFIED
Department of Energy (DOE)DE-AC02-07CH11359
Ministerio de Educación y Ciencia (MEC)UNSPECIFIED
University of NottinghamUNSPECIFIED
NSFAST-1138766
NSFAST-1536171
Issue or Number:10
DOI:10.1103/physrevd.105.103537
Record Number:CaltechAUTHORS:20220608-849415000
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20220608-849415000
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:115084
Collection:CaltechAUTHORS
Deposited By: George Porter
Deposited On:14 Jun 2022 16:19
Last Modified:25 Jul 2022 23:14

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