Joint analysis of Dark Energy Survey Year 3 data and CMB lensing from SPT and<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mi>P</mml:mi><mml:mi>l</mml:mi><mml:mi>a</mml:mi><mml:mi>n</mml:mi><mml:mi>c</mml:mi><mml:mi>k</mml:mi></mml:mrow></mml:math>. II. Cross-correlation measurements and cosmological constraints
C. ChangArgonne National Laboratory, 9700 South Cass Avenue, Lemont, Illinois 60439, USAY. OmoriDepartment of Astronomy and Astrophysics, University of Chicago, Chicago, Illinois 60637, USAEric J. BaxterInstitute for Astronomy, University of Hawai‘i, 2680 Woodlawn Drive, Honolulu, Hawaii 96822, USAC. DouxDepartment of Physics and Astronomy, University of Pennsylvania, Philadelphia, Pennsylvania 19104, USAA. ChoiCalifornia Institute of Technology, 1200 East California Blvd, MC 249-17, Pasadena, California 91125, USAS. PandeyDepartment of Physics and Astronomy, University of Pennsylvania, Philadelphia, Pennsylvania 19104, USAA. AlarconArgonne National Laboratory, 9700 South Cass Avenue, Lemont, Illinois 60439, USAO. AlvesDepartment of Physics, University of Michigan, Ann Arbor, Michigan 48109, USAA. AmonKavli Institute for Particle Astrophysics & Cosmology, P. O. Box 2450, Stanford University, Stanford, California 94305, USAF. Andrade-OliveiraDepartment of Physics, University of Michigan, Ann Arbor, Michigan 48109, USAK. BechtolPhysics Department, 2320 Chamberlin Hall, University of Wisconsin-Madison, 1150 University Avenue Madison, Wisconsin 53706-1390M. R. BeckerArgonne National Laboratory, 9700 South Cass Avenue, Lemont, Illinois 60439, USAG. M. BernsteinDepartment of Physics and Astronomy, University of Pennsylvania, Philadelphia, Pennsylvania 19104, USAF. BianchiniDepartment of Physics, Stanford University, 382 Via Pueblo Mall, Stanford, California 94305, USAJ. BlazekDepartment of Physics, Northeastern University, Boston, Massachusetts 02115, USAL. E. BleemArgonne National Laboratory, 9700 South Cass Avenue, Lemont, Illinois 60439, USAH. CamachoInstituto de Física Teórica, Universidade Estadual Paulista, São Paulo, BrazilA. CamposDepartment of Physics, Carnegie Mellon University, Pittsburgh, Pennsylvania 15312, USAA. 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 St., Urbana, Illinois 61801, USAR. CawthonPhysics Department, William Jewell College, Liberty, Missouri, 64068R. ChenDepartment of Physics, Duke University Durham, North Carolina 27708, USAJ. CorderoJodrell Bank Center for Astrophysics, School of Physics and Astronomy, University of Manchester, Oxford Road, Manchester, M13 9PL, United KingdomT. M. CrawfordDepartment of Astronomy and Astrophysics, University of Chicago, Chicago, Illinois 60637, USAM. CrocceInstitut d’Estudis Espacials de Catalunya (IEEC), 08034 Barcelona, SpainC. DavisKavli Institute for Particle Astrophysics & Cosmology, P. O. Box 2450, Stanford University, Stanford, California 94305, USAJ. DeRoseLawrence Berkeley National Laboratory, 1 Cyclotron Road, Berkeley, California 94720, USAScott DodelsonDepartment of Physics, Carnegie Mellon University, Pittsburgh, Pennsylvania 15312, USAA. Drlica-WagnerDepartment of Astronomy and Astrophysics, University of Chicago, Chicago, Illinois 60637, USAK. EckertDepartment of Physics and Astronomy, University of Pennsylvania, Philadelphia, Pennsylvania 19104, USAT. F. EiflerDepartment of Astronomy/Steward Observatory, University of Arizona, 933 North Cherry Avenue, Tucson, Arizona 85721-0065, USAF. ElsnerDepartment of Physics & Astronomy, University College London, Gower Street, London, WC1E 6BT, United KingdomJ. Elvin-PooleCenter for Cosmology and Astro-Particle Physics, The Ohio State University, Columbus, Ohio 43210, USAS. EverettXiao FangDepartment of Astronomy, University of California, Berkeley, 501 Campbell Hall, Berkeley, California 94720, USAA. FertéJet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, California 91109, USAP. FosalbaInstitut d’Estudis Espacials de Catalunya (IEEC), 08034 Barcelona, SpainO. FriedrichKavli Institute for Cosmology, University of Cambridge, Madingley Road, Cambridge CB3 0HA, United KingdomM. GattiDepartment of Physics and Astronomy, University of Pennsylvania, Philadelphia, Pennsylvania 19104, USAG. GianniniInstitut de Física d’Altes Energies (IFAE), The Barcelona Institute of Science and Technology, Campus UAB, 08193 Bellaterra (Barcelona) SpainD. GruenUniversity Observatory, Faculty of Physics, Ludwig-Maximilians-Universitat, Scheinerstrasse 1, 81679 Munich, GermanyR. A. GruendlCenter for Astrophysical Surveys, National Center for Supercomputing Applications, 1205 West Clark St., Urbana, Illinois 61801, USAI. HarrisonDepartment of Physics, University of Oxford, Denys Wilkinson Building, Keble Road, Oxford OX1 3RH, United KingdomK. HernerFermi National Accelerator Laboratory, P. O. Box 500, Batavia, Illinois 60510, USAH. HuangDepartment of Astronomy/Steward Observatory, University of Arizona, 933 North Cherry Avenue, Tucson, Arizona 85721-0065, USAEric HuffJet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, California 91109, USADragan HutererDepartment of Physics, University of Michigan, Ann Arbor, Michigan 48109, USAMike JarvisDepartment of Physics and Astronomy, University of Pennsylvania, Philadelphia, Pennsylvania 19104, USAAndrás KovácsInstituto de Astrofisica de Canarias, E-38205 La Laguna, Tenerife, SpainE. KrauseDepartment of Astronomy/Steward Observatory, University of Arizona, 933 North Cherry Avenue, Tucson, Arizona 85721-0065, USAN. KuropatkinFermi National Accelerator Laboratory, P. O. Box 500, Batavia, Illinois 60510, USAP. -F. LegetKavli Institute for Particle Astrophysics & Cosmology, P. O. Box 2450, Stanford University, Stanford, California 94305, USAPablo LemosDepartment of Physics & Astronomy, University College London, Gower Street, London, WC1E 6BT, United KingdomAndrew R. LiddleInstituto de Astrofísica e Ciências do Espaço, Faculdade de Ciências, Universidade de Lisboa, 1769-016 Lisboa, PortugalN. MacCrannDepartment of Applied Mathematics and Theoretical Physics, University of Cambridge, Cambridge CB3 0WA, United KingdomJ. McCulloughKavli Institute for Particle Astrophysics & Cosmology, P. O. Box 2450, Stanford University, Stanford, California 94305, USAJ. MuirPerimeter Institute for Theoretical Physics, 31 Caroline St. North, Waterloo, Ontario N2L 2Y5, CanadaJ. 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, SP, BrazilY. ParkKavli Institute for the Physics and Mathematics of the Universe (WPI), UTIAS, The University of Tokyo, Kashiwa, Chiba 277-8583, JapanA. PorredonCenter for Cosmology and Astro-Particle Physics, The Ohio State University, Columbus, Ohio 43210, USAJ. PratDepartment of Astronomy and Astrophysics, University of Chicago, Chicago, Illinois 60637, USAMarco RaveriDepartment of Physics and Astronomy, University of Pennsylvania, Philadelphia, Pennsylvania 19104, USAR. P. RollinsJodrell Bank Center for Astrophysics, School of Physics and Astronomy, University of Manchester, Oxford Road, Manchester, M13 9PL, United KingdomA. RoodmanKavli Institute for Particle Astrophysics & Cosmology, P. O. Box 2450, Stanford University, Stanford, California 94305, USAR. RosenfeldICTP South American Institute for Fundamental Research Instituto de Física Teórica, Universidade Estadual Paulista, São Paulo, BrazilA.J. RossCenter for Cosmology and Astro-Particle Physics, The Ohio State University, Columbus, Ohio 43210, USAE. S. RykoffKavli Institute for Particle Astrophysics & Cosmology, P. O. Box 2450, Stanford University, Stanford, California 94305, USAC. SánchezDepartment of Physics and Astronomy, University of Pennsylvania, Philadelphia, Pennsylvania 19104, USAJ. SanchezFermi National Accelerator Laboratory, P. O. Box 500, Batavia, Illinois 60510, USAL. F. SeccoKavli Institute for Cosmological Physics, University of Chicago, Chicago, Illinois 60637, USAI. Sevilla-NoarbeCentro de Investigaciones Energéticas, Medioambientales y Tecnológicas (CIEMAT), Madrid, SpainE. SheldonBrookhaven National Laboratory, Bldg 510, Upton, New York 11973, USAT. ShinDepartment of Physics and Astronomy, University of Pennsylvania, Philadelphia, Pennsylvania 19104, USAM. A. TroxelDepartment of Physics, Duke University Durham, North Carolina 27708, USAI. TutusausDépartement de Physique Théorique and Center for Astroparticle Physics, Université de Genève, 24 quai Ernest Ansermet, CH-1211 Geneva, SwitzerlandT. N. VargaMax Planck Institute for Extraterrestrial Physics, Giessenbachstrasse, 85748 Garching, GermanyN. WeaverdyckDepartment of Physics, University of Michigan, Ann Arbor, Michigan 48109, USAR.H. WechslerDepartment of Physics, Stanford University, 382 Via Pueblo Mall, Stanford, California 94305, USAW. L. K. WuKavli Institute for Particle Astrophysics & Cosmology, P. O. Box 2450, Stanford University, Stanford, California 94305, USAB. YannyFermi National Accelerator Laboratory, P. O. Box 500, Batavia, Illinois 60510, USAB. YinDepartment of Physics, Carnegie Mellon University, Pittsburgh, Pennsylvania 15312, USAY. ZhangFermi National Accelerator Laboratory, P. O. Box 500, Batavia, Illinois 60510, USAJ. ZuntzInstitute for Astronomy, University of Edinburgh, Edinburgh EH9 3HJ, United KingdomT. 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, USAJ. AnnisFermi National Accelerator Laboratory, P. O. Box 500, Batavia, Illinois 60510, USAD. BaconInstitute of Cosmology and Gravitation, University of Portsmouth, Portsmouth, PO1 3FX, United KingdomB. A. BensonDepartment of Astronomy and Astrophysics, University of Chicago, Chicago, Illinois 60637, USAE. BertinCNRS, UMR 7095, Institut d’Astrophysique de Paris, F-75014, Paris, FranceS. BocquetLudwig-Maximilians-Universität, Scheiner- strasse 1, 81679 Munich, GermanyD. BrooksDepartment of Physics & Astronomy, University College London, Gower Street, London, WC1E 6BT, United KingdomD. L. BurkeKavli Institute for Particle Astrophysics & Cosmology, P. O. Box 2450, Stanford University, Stanford, California 94305, USAJ. E. CarlstromArgonne National Laboratory, 9700 South Cass Avenue, Lemont, Illinois 60439, USAJ. CarreteroInstitut de Física d’Altes Energies (IFAE), The Barcelona Institute of Science and Technology, Campus UAB, 08193 Bellaterra (Barcelona) SpainC. L. ChangArgonne National Laboratory, 9700 South Cass Avenue, Lemont, Illinois 60439, USARyan ChownDepartment of Physics & Astronomy, The University of Western Ontario, London Ontario N6A 3K7, CanadaM. CostanziAstronomy Unit, Department of Physics, University of Trieste, via Tiepolo 11, I-34131 Trieste, ItalyL. N. da CostaLaboratório Interinstitucional de e-Astronomia - LIneA, Rua Gal. José Cristino 77, Rio de Janeiro, RJ - 20921-400, Brazil
2023lv
ABI
Abstract
Cross-correlations of galaxy positions and galaxy shears with maps of gravitational lensing of the cosmic microwave background (CMB) are sensitive to the distribution of large-scale structure in the Universe. Such cross-correlations are also expected to be immune to some of the systematic effects that complicate correlation measurements internal to galaxy surveys. We present measurements and modeling of the cross-correlations between galaxy positions and galaxy lensing measured in the first three years of data from the Dark Energy Survey with CMB lensing maps derived from a combination of data from the 2500 deg2 SPT-SZ survey conducted with the South Pole Telescope and full-sky data from the Planck satellite. The CMB lensing maps used in this analysis have been constructed in a way that minimizes biases from the thermal Sunyaev Zel'dovich effect, making them well suited for cross-correlation studies. The total signal-to-noise of the cross-correlation measurements is 23.9 (25.7) when using a choice of angular scales optimized for a linear (nonlinear) galaxy bias model. We use the cross-correlation measurements to obtain constraints on cosmological parameters. For our fiducial galaxy sample, which consist of four bins of magnitude-selected galaxies, we find constraints of omega m 1/4 0.272 thorn 0.032 pffiffiffiffiffiffiffiffiffiffiffiffiffiffi-0.052 and S8 equivalent to sigma 8 omega m=0.3 1/4 0.736 thorn 0.032 -0.028 (omega m 1/40.245 thorn 0.0-0.04426 and S8 1/40.734 thorn 0.035 -0.028 ) when assuming linear (nonlinear) galaxy bias in our modeling. Considering only the cross-correlation of galaxy shear with CMB lensing, we find omega m 1/4 0.270 thorn 0.043 -0.061 and S8 1/4 0.740 thorn 0.034 -0.029 . Our constraints on S8 are consistent with recent cosmic shear measurements, but lower than the values preferred by primary CMB measurements from Planck.
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Cited by 20 references