Cross-correlation of Dark Energy Survey Year 3 lensing data with ACT and <i>Planck</i> thermal Sunyaev-Zel’dovich effect observations. I. Measurements, systematics tests, and feedback model constraints
M. GattiDepartment of Physics and Astronomy, University of Pennsylvania, Philadelphia, Pennsylvania 19104, USAShivam PandeyDepartment of Physics and Astronomy, University of Pennsylvania, Philadelphia, Pennsylvania 19104, USAEric J. BaxterInstitute for Astronomy, University of Hawai’i, 2680 Woodlawn Drive, Honolulu, Hawai’i 96822, USAJ. Colin HillCenter for Computational Astrophysics, Flatiron Institute, New York, New York 10010, USAE. Barry MoserDepartment of Astronomy, Cornell University, Ithaca, New York 14853, USAMarco RaveriDepartment of Physics and Astronomy, University of Pennsylvania, Philadelphia, Pennsylvania 19104, USAXiao FangDepartment of Astronomy/Steward Observatory, University of Arizona, 933 North Cherry Avenue, Tucson, Arizona 85721-0065, USAJ. DeRoseLawrence Berkeley National Laboratory, 1 Cyclotron Road, Berkeley, California 94720, USAG. GianniniInstitut de Física d’Altes Energies (IFAE), The Barcelona Institute of Science and Technology, Campus UAB, 08193 Bellaterra (Barcelona), SpainC. DouxDepartment of Physics and Astronomy, University of Pennsylvania, Philadelphia, Pennsylvania 19104, USAHung-Jin HuangDepartment of Physics, University of Arizona, Tucson, Arizona 85721, USANicholas BattagliaDepartment of Astronomy, Cornell University, Ithaca, New York 14853, USAA. AlarconArgonne National Laboratory, 9700 South Cass Avenue, Lemont, Illinois 60439, USAA. AmonKavli Institute for Particle Astrophysics and Cosmology, P. O. Box 2450, Stanford University, Stanford, California 94305, USAM. R. BeckerArgonne National Laboratory, 9700 South Cass Avenue, Lemont, Illinois 60439, USAA. CamposDepartment of Physics, Carnegie Mellon University, Pittsburgh, Pennsylvania 15312, USAC. ChangDepartment of Astronomy and Astrophysics, University of Chicago, Chicago, Illinois 60637, USAR. ChenDepartment of Physics, Duke University, Durham, North Carolina 27708, USAA. ChoiCenter for Cosmology and Astro-Particle Physics, The Ohio State University, Columbus, Ohio 43210, USAK. EckertDepartment of Physics and Astronomy, University of Pennsylvania, Philadelphia, Pennsylvania 19104, USAJ. Elvin-PooleCenter for Cosmology and Astro-Particle Physics, The Ohio State University, Columbus, Ohio 43210, USAS. EverettA. FertéJet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, California 91109, USAI. HarrisonDepartment of Physics, University of Oxford, Denys Wilkinson Building, Keble Road, Oxford OX1 3RH, United KingdomN. MacCrannDepartment of Applied Mathematics and Theoretical Physics, University of Cambridge, Cambridge CB3 0WA, United KingdomJ. McCulloughKavli Institute for Particle Astrophysics and Cosmology, P. O. Box 2450, Stanford University, Stanford, California 94305, USAJ. MylesDepartment of Physics, Stanford University, 382 Via Pueblo Mall, Stanford, California 94305, USAA Navarro-AlsinaInstituto de Física Gleb Wataghin, Universidade Estadual de Campinas, 13083-859 Campinas, São Paulo, BrazilJ. PratDepartment of Astronomy and Astrophysics, University of Chicago, Chicago, Illinois 60637, USAR. P. RollinsJodrell Bank Center for Astrophysics, School of Physics and Astronomy, University of Manchester, Oxford Road, Manchester M13 9PL, United KingdomC. SánchezDepartment of Physics and Astronomy, University of Pennsylvania, Philadelphia, Pennsylvania 19104, USAT. ShinDepartment of Physics and Astronomy, University of Pennsylvania, Philadelphia, Pennsylvania 19104, USAM. A. TroxelDepartment of Physics, Duke University, Durham, North Carolina 27708, USAI. TutusausInstitut d’Estudis Espacials de Catalunya (IEEC), 08034 Barcelona, SpainB. YinDepartment of Physics, Carnegie Mellon University, Pittsburgh, Pennsylvania 15312, USAT. M. C. AbbottCerro Tololo Inter-American Observatory, NSF’s National Optical-Infrared Astronomy Research Laboratory, Casilla 603, La Serena, ChileM. AguenaLaboratório Interinstitucional de e-Astronomia - LIneA, Rua Gal. José Cristino 77, Rio de Janeiro, RJ - 20921-400, BrazilS. AllamFermi National Accelerator Laboratory, P. O. Box 500, Batavia, Illinois 60510, USAF. Andrade-OliveiraInstituto de Física Teórica, Universidade Estadual Paulista, 01140-070 São Paulo, BrazilJ. AnnisFermi National Accelerator Laboratory, P. O. Box 500, Batavia, Illinois 60510, USAG. M. BernsteinDepartment of Physics and Astronomy, University of Pennsylvania, Philadelphia, Pennsylvania 19104, USAE. BertinCNRS, UMR 7095, Institut d’Astrophysique de Paris, F-75014 Paris, FranceBoris BollietDepartment of Physics, Columbia University, New York, New York 10027, USAJ. R. BondCanadian Institute for Theoretical Astrophysics, 60 St. George Street, University of Toronto, Toronto, Ontario M5S 3H8, CanadaDavid BrooksDepartment of Physics and Astronomy, University College London, Gower Street, London WC1E 6BT, United KingdomD. L. BurkeKavli Institute for Particle Astrophysics and Cosmology, P. O. Box 2450, Stanford University, Stanford, California 94305, USAErminia CalabreseSchool of Physics and Astronomy, Cardiff University, The Parade, Cardiff CF24 3AA, United KingdomA. Carnero RosellInstituto de Astrofisica de Canarias, E-38205 La Laguna, Tenerife, SpainM. Carrasco KindCenter for Astrophysical Surveys, National Center for Supercomputing Applications, 1205 West Clark Street, Urbana, Illinois 61801, USAJ. CarreteroInstitut de Física d’Altes Energies (IFAE), The Barcelona Institute of Science and Technology, Campus UAB, 08193 Bellaterra (Barcelona), SpainR. CawthonPhysics Department, 2320 Chamberlin Hall, University of Wisconsin-Madison, 1150 University Avenue, Madison, Wisconsin 53706-1390, USAM. CostanziAstronomy Unit, Department of Physics, University of Trieste, via Tiepolo 11, I-34131 Trieste, ItalyM. CrocceInstitut d’Estudis Espacials de Catalunya (IEEC), 08034 Barcelona, SpainL. N. da CostaLaboratório Interinstitucional de e-Astronomia - LIneA, Rua Gal. José Cristino 77, Rio de Janeiro, RJ - 20921-400, BrazilM. E. S. PereiraDepartment of Physics, University of Michigan, Ann Arbor, Michigan 48109, USAJ. De VicenteCentro de Investigaciones Energéticas, Medioambientales y Tecnológicas (CIEMAT), 28040 Madrid, SpainS. DesaiDepartment of Physics, IIT Hyderabad, Kandi, Telangana 502285, IndiaH. T. DiehlFermi National Accelerator Laboratory, P. O. Box 500, Batavia, Illinois 60510, USAJ. P. DietrichFaculty of Physics, Ludwig-Maximilians-Universität, Scheinerstrasse 1, 81679 Munich, GermanyP. DoelDepartment of Physics and Astronomy, University College London, Gower Street, London WC1E 6BT, United KingdomJo DunkleyDepartment of Astrophysical Sciences, Princeton University, Peyton Hall, Princeton, New Jersey 08544, USAA. E. EvrardDepartment of Astronomy, University of Michigan, Ann Arbor, Michigan 48109, USAS. FerraroBerkeley Center for Cosmological Physics, University of California, Berkeley, California 94720, USAI. FerreroInstitute of Theoretical Astrophysics, University of Oslo, P.O. Box 1029 Blindern, NO-0315 Oslo, NorwayB. FlaugherFermi National Accelerator Laboratory, P. O. Box 500, Batavia, Illinois 60510, USAP. FosalbaInstitut d’Estudis Espacials de Catalunya (IEEC), 08034 Barcelona, SpainJ. García-BellidoInstituto de Fisica Teorica UAM/CSIC, Universidad Autonoma de Madrid, 28049 Madrid, SpainE. GaztañagaInstitut d’Estudis Espacials de Catalunya (IEEC), 08034 Barcelona, SpainD. W. GerdesDepartment of Astronomy, University of Michigan, Ann Arbor, Michigan 48109, USAT. GiannantonioInstitute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 0HA, United KingdomD. GruenFaculty of Physics, Ludwig-Maximilians-Universität, Scheinerstrasse 1, 81679 Munich, GermanyR. A. GruendlCenter for Astrophysical Surveys, National Center for Supercomputing Applications, 1205 West Clark Street, Urbana, Illinois 61801, USAJ. GschwendLaboratório Interinstitucional de e-Astronomia - LIneA, Rua Gal. José Cristino 77, Rio de Janeiro, RJ - 20921-400, BrazilG. GutiérrezFermi National Accelerator Laboratory, P. O. Box 500, Batavia, Illinois 60510, USAK. HernerFermi National Accelerator Laboratory, P. O. Box 500, Batavia, Illinois 60510, USAAdam D. HincksDavid A. Dunlap Department of Astronomy and Astrophysics, University of Toronto, 50 St. George Street, Toronto, Ontario M5S 3H4, CanadaS. R. HintonSchool of Mathematics and Physics, University of Queensland, Brisbane, Queensland 4072, AustraliaD. L. HollowoodK. HonscheidCenter for Cosmology and Astro-Particle Physics, The Ohio State University, Columbus, Ohio 43210, USAJohn P. HughesDepartment of Physics and Astronomy, Rutgers, the State University of New Jersey, 136 Frelinghuysen Road, Piscataway, New Jersey 08854-8019, USADragan HutererDepartment of Physics, University of Michigan, Ann Arbor, Michigan 48109, USABhuvnesh JainDepartment of Physics and Astronomy, University of Pennsylvania, Philadelphia, Pennsylvania 19104, USAD. J. JamesCenter for Astrophysics | Harvard and Smithsonian, 60 Garden Street, Cambridge, Massachusetts 02138, USAE. KrauseDepartment of Astronomy/Steward Observatory, University of Arizona, 933 North Cherry Avenue, Tucson, Arizona 85721-0065, USAK. KuehnAustralian Astronomical Optics, Macquarie University, North Ryde, New South Wales 2113, AustraliaN. KuropatkinFermi National Accelerator Laboratory, P. O. Box 500, Batavia, Illinois 60510, USAO. LahavDepartment of Physics and Astronomy, University College London, Gower Street, London WC1E 6BT, United KingdomC. LidmanCentre for Gravitational Astrophysics, College of Science, The Australian National University, Australian Capital Territory 2601, AustraliaM. LimaDepartamento de Física Matemática, Instituto de Física, Universidade de São Paulo, CP 66318, São Paulo, SP 05314-970, BrazilMartine LokkenCanadian Institute for Theoretical Astrophysics, 60 St. George Street, University of Toronto, Toronto, Ontario M5S 3H8, CanadaMathew S. MadhavacherilPerimeter Institute for Theoretical Physics, 31 Caroline Street North, Waterloo, Ontario N2L 2Y5, CanadaM. A. G. MaiaLaboratório Interinstitucional de e-Astronomia - LIneA, Rua Gal. José Cristino 77, Rio de Janeiro, RJ - 20921-400, BrazilJ. L. MarshallDepartment of Physics and Astronomy, George P. and Cynthia Woods Mitchell Institute for Fundamental Physics and Astronomy, Texas A&M University, College Station, Texas 77843, USAJ. J. McMahonDepartment of Astronomy and Astrophysics, University of Chicago, 5640 South Ellis Avenue, Chicago, Illinois 60637, USAP. MelchiorDepartment of Astrophysical Sciences, Princeton University, Peyton Hall, Princeton, New Jersey 08544, USAKavilan MoodleyAstrophysics Research Centre, University of KwaZulu-Natal, Westville Campus, Durban 4041, South AfricaJ. J. MohrFaculty of Physics, Ludwig-Maximilians-Universität, Scheinerstrasse 1, 81679 Munich, GermanyR. MorganPhysics Department, 2320 Chamberlin Hall, University of Wisconsin-Madison, 1150 University Avenue, Madison, Wisconsin 53706-1390, USAF. NatiDepartment of Physics, University of Milano-Bicocca, Piazza della Scienza 3, 20126 Milano (MI), Italy
2022en
ABI
Аннотация
We present a tomographic measurement of the cross-correlation between thermal Sunyaev-Zel'dovich (TSZ) maps from Planck and the Atacama Cosmology Telescope and weak galaxy lensing shears measured during the first three years of observations of the Dark Energy Survey. This correlation is sensitive to the thermal energy in baryons over a wide redshift range and is therefore a powerful probe of astrophysical feedback. We detect the correlation at a statistical significance of $21\ensuremath{\sigma}$, the highest significance to date. We examine the TSZ maps for potential contaminants, including cosmic infrared background and radio sources, finding that cosmic infrared background has a substantial impact on our measurements and must be taken into account in our analysis. We use the cross-correlation measurements to test different feedback models. In particular, we model the TSZ using several different pressure profile models calibrated against hydrodynamical simulations. Our analysis marginalizes over redshift uncertainties, shear calibration biases, and intrinsic alignment effects. We also marginalize over ${\mathrm{\ensuremath{\Omega}}}_{\mathrm{m}}$ and ${\ensuremath{\sigma}}_{8}$ using Planck or DES priors. We find that the data prefer the model with a low amplitude of the pressure profile at small scales, compatible with a scenario with strong active galactic nuclei feedback and ejection of gas from the inner part of the halos. When using a more flexible model for the shear profile, constraints are weaker, and the data cannot discriminate between different baryonic prescriptions.
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