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Title: Weak-lensing analysis of SPT-selected galaxy clusters using Dark Energy Survey Science Verification data

Journal Article · · Monthly Notices of the Royal Astronomical Society
DOI:https://doi.org/10.1093/mnras/stz234· OSTI ID:1504477
 [1];  [1];  [2];  [3];  [4];  [5];  [6];  [7];  [8];  [9];  [10];  [11];  [12];  [13];  [14];  [1];  [1];  [15];  [16];  [17] more »;  [18];  [19];  [1];  [20];  [21];  [22];  [23];  [24];  [7];  [25];  [26];  [27];  [8];  [25];  [28];  [29];  [30];  [24];  [30];  [31];  [30];  [27];  [32];  [33];  [27];  [6];  [25];  [30];  [34];  [34];  [24];  [35];  [30];  [24];  [36];  [25];  [8];  [37];  [6];  [38];  [39];  [40];  [29];  [41];  [42];  [29];  [43];  [20];  [44];  [45];  [46];  [42];  [20] « less
  1. Faculty of Physics, Ludwig-Maximilians-Universität, Scheinerstr. 1, D-81679 Munich, Germany; Excellence Cluster Universe, Boltzmannstr. 2, D-85748 Garching, Germany
  2. Argonne National Laboratory, 9700 South Cass Avenue, Lemont, IL 60439, USA
  3. Kavli Institute for Cosmological Physics, University of Chicago, 5640 South Ellis Avenue, Chicago, IL 60637, USA; Argelander-Institut für Astronomie, Universität Bonn, Auf dem Hügel 71, D-53121, Bonn, Germany
  4. Faculty of Physics, Ludwig-Maximilians-Universität, Scheinerstr. 1, D-81679 Munich, Germany; Excellence Cluster Universe, Boltzmannstr. 2, D-85748 Garching, Germany; Max Planck Institute for Extraterrestrial Physics, Giessenbachstrasse, D-85748 Garching, Germany
  5. Jodrell Bank Center for Astrophysics, School of Physics and Astronomy, University of Manchester, Oxford Road, Manchester M13 9PL, UK
  6. Department of Astronomy, University of Illinois at Urbana-Champaign, 1002 W. Green Street, Urbana, IL 61801, USA; National Center for Supercomputing Applications, 1205 West Clark Str, Urbana, IL 61801, USA
  7. Kavli Institute for Particle Astrophysics & Cosmology, PO Box 2450, Stanford University, Stanford, CA 94305, USA; SLAC National Accelerator Laboratory, Menlo Park, CA 94025, USA
  8. Department of Physics and Astronomy, University of Pennsylvania, Philadelphia, PA 19104, USA
  9. Department of Physics, ETH Zurich, Wolfgang-Pauli-Strasse 16, CH-8093 Zurich, Switzerland
  10. Faculty of Physics, Ludwig-Maximilians-Universität, Scheinerstr. 1, D-81679 Munich, Germany; INAF-Osservatorio Astronomico di Trieste, via G. B. Tiepolo 11, I-34143 Trieste, Italy
  11. Brookhaven National Laboratory, Bldg 510, Upton, NY 11973, USA
  12. Center for Cosmology and Astro-Particle Physics, The Ohio State University, Columbus, OH 43210, USA; Department of Physics, The Ohio State University, Columbus, OH 43210, USA
  13. Institute for Astronomy, University of Edinburgh, Edinburgh EH9 3HJ, UK
  14. Fermi National Accelerator Laboratory, PO Box 500, Batavia, IL 60510, USA; Department of Astronomy and Astrophysics, University of Chicago, 5640 South Ellis Avenue, Chicago, IL 60637; Kavli Institute for Cosmological Physics, University of Chicago, Chicago, IL 60637, USA
  15. Department of Physics, IIT Hyderabad, Kandi, Telangana 502285, India
  16. Center for Astrophysics and Space Astronomy, Department of Astrophysical and Planetary Science, University of Colorado, Boulder, C0 80309, USA; NASA Ames Research Center, Moffett Field, CA 94035, USA
  17. School of Physics, University of Melbourne, Parkville, VIC 3010, Australia
  18. Physics Department, Case Western Reserve University, Cleveland, Ohio 44106, USA; Department of Physics, Yale University, New Haven, CT 06511, USA
  19. Argelander-Institut für Astronomie, Universität Bonn, Auf dem Hügel 71, D-53121, Bonn, Germany
  20. Cerro Tololo Inter-American Observatory, National Optical Astronomy Observatory, Casilla 603, La Serena, Chile
  21. Department of Physics & Astronomy, University College London, Gower Street, London, WC1E 6BT, UK; Department of Physics and Electronics, Rhodes University, PO Box 94, Grahamstown, 6140, South Africa
  22. Institute of Cosmology & Gravitation, University of Portsmouth, Portsmouth PO1 3FX, UK
  23. CNRS, UMR 7095, Institut d’Astrophysique de Paris, F-75014, Paris, France; Sorbonne Universités, UPMC Univ Paris 06, UMR 7095, Institut d’Astrophysique de Paris, F-75014, Paris, France
  24. Department of Physics & Astronomy, University College London, Gower Street, London, WC1E 6BT, UK
  25. Laboratório Interinstitucional de e-Astronomia - LIneA, Rua Gal. José Cristino 77, Rio de Janeiro, RJ - 20921-400, Brazil; Observatório Nacional, Rua Gal. José Cristino 77, Rio de Janeiro, RJ - 20921-400, Brazil
  26. Institut de Física d’Altes Energies (IFAE), The Barcelona Institute of Science and Technology, Campus UAB, E-08193 Bellaterra (Barcelona), Spain
  27. Institut d’Estudis Espacials de Catalunya (IEEC), E-08193 Barcelona, Spain; Institute of Space Sciences (ICE, CSIC), Campus UAB, Carrer de Can Magrans, s/n, E-08193 Barcelona, Spain
  28. Kavli Institute for Particle Astrophysics & Cosmology, PO Box 2450, Stanford University, Stanford, CA 94305, USA
  29. Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas (CIEMAT), 28040 Madrid, Spain
  30. Fermi National Accelerator Laboratory, PO Box 500, Batavia, IL 60510, USA
  31. Department of Astronomy, University of Michigan, Ann Arbor, MI 48109, USA; Department of Physics, University of Michigan, Ann Arbor, MI 48109, USA
  32. Fermi National Accelerator Laboratory, PO Box 500, Batavia, IL 60510, USA; Kavli Institute for Cosmological Physics, University of Chicago, Chicago, IL 60637, USA
  33. Instituto de Fisica Teorica UAM/CSIC, Universidad Autonoma de Madrid, E-28049 Madrid, Spain
  34. Santa Cruz Institute for Particle Physics, Santa Cruz, CA 95064, USA
  35. Australian Astronomical Observatory, North Ryde, NSW 2113, Australia
  36. Laboratório Interinstitucional de e-Astronomia - LIneA, Rua Gal. José Cristino 77, Rio de Janeiro, RJ - 20921-400, Brazil; Departamento de Física Matemática, Instituto de Física, Universidade de São Paulo, CP 66318, São Paulo, SP 05314-970, Brazil
  37. Department of Astrophysical Sciences, Princeton University, Peyton Hall, Princeton, NJ 08544, USA
  38. Institut de Física d’Altes Energies (IFAE), The Barcelona Institute of Science and Technology, Campus UAB, E-08193 Bellaterra (Barcelona), Spain; Institució Catalana de Recerca i Estudis Avançats, E-08010 Barcelona, Spain
  39. Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Dr., Pasadena, CA 91109, USA
  40. Department of Physics and Astronomy, Pevensey Building, University of Sussex, Brighton BN1 9QH, UK
  41. SLAC National Accelerator Laboratory, Menlo Park, CA 94025, USA
  42. Department of Physics, University of Michigan, Ann Arbor, MI 48109, USA
  43. School of Physics and Astronomy, University of Southampton, Southampton SO17 1BJ, UK
  44. Laboratório Interinstitucional de e-Astronomia - LIneA, Rua Gal. José Cristino 77, Rio de Janeiro, RJ - 20921-400, Brazil; Instituto de Física Gleb Wataghin, Universidade Estadual de Campinas, Campinas, SP13083-859, Brazil
  45. Computer Science and Mathematics Division, Oak Ridge National Laboratory, Oak Ridge, TN 37831, USA
  46. National Center for Supercomputing Applications, 1205 West Clark Str, Urbana, IL 61801, USA

Here, we present weak lensing (WL) mass constraints for a sample of massive galaxy clusters detected by the South Pole Telescope (SPT) via the Sunyaev-Zel'dovich effect (SZE). We use griz imaging data obtained from the Science Verification (SV) phase of the Dark Energy Survey (DES) to fit the WL shear signal of 33 clusters in the redshift range 0.25 ≤ z ≤ 0.8 with NFW profiles and to constrain a four-parameter SPT mass-observable relation. To account for biases in WL masses, we introduce a WL mass to true mass scaling relation described by a mean bias and an intrinsic, log-normal scatter. We allow for correlated scatter within the WL and SZE mass-observable relations and use simulations to constrain priors on nuisance parameters related to bias and scatter from WL. We constrain the normalization of the $$\zeta$$-M500 relation, $$\mathrm{A_{SZ}}$$ = 12.0$$+2.6\atop{-6.7}$$ when using a prior on the mass slope $$B_\mathrm{SZ}$$ from the latest SPT cluster cosmology analysis. Without this prior, we recover $$A_\mathrm{SZ}=10.8_{-5.2}^{+2.3}$$ and $$B_\mathrm{SZ}=1.30_{-0.44}^{+0.22}$$. Results in both cases imply lower cluster masses than measured in previous work with and without WL, although the uncertainties are large. The WL derived value of $$B_\mathrm{SZ}$$ is $$\approx 20\%$$ lower than the value preferred by the most recent SPT cluster cosmology analysis. The method shown in this work is designed to constrain cluster masses and cosmological parameters simultaneously and will form the basis for subsequent studies that employ the full SPT cluster sample together with the DES data.

Research Organization:
Brookhaven National Laboratory (BNL), Upton, NY (United States); SLAC National Accelerator Laboratory (SLAC), Menlo Park, CA (United States); Fermi National Accelerator Laboratory (FNAL), Batavia, IL (United States); Oak Ridge National Laboratory (ORNL), Oak Ridge, TN (United States); Univ. of Michigan, Ann Arbor, MI (United States)
Sponsoring Organization:
USDOE Office of Science (SC), High Energy Physics (HEP); USDOE Office of Science (SC), Advanced Scientific Computing Research (ASCR)
Contributing Organization:
DES & SPT Collaborations; DES and SPT Collaborations
Grant/Contract Number:
AC02-07CH11359; SC0019193; AC05-00OR22725
OSTI ID:
1504477
Alternate ID(s):
OSTI ID: 1505306; OSTI ID: 1725794
Report Number(s):
arXiv:1802.04533; DES 2016-0159; FERMILAB-PUB-17-026-AE; oai:inspirehep.net:1654864
Journal Information:
Monthly Notices of the Royal Astronomical Society, Vol. 485, Issue 1; ISSN 0035-8711
Publisher:
Royal Astronomical SocietyCopyright Statement
Country of Publication:
United States
Language:
English
Citation Metrics:
Cited by: 20 works
Citation information provided by
Web of Science

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