SPT clusters with DES and HST weak lensing. II. Cosmological constraints from the abundance of massive halos

In these two papers, the authors use mock maps to establish a method for studying the abundance and calibrating the weak-lensing based mass of galaxy clusters. They set up a likelihood function, thus obtaining cosmological constraints from a sample of 1,005 clusters detected with the South Pole Telescope, in combination with further cluster data from the Dark Energy Survey, the Wide-field Infrared Survey Explorer, and the Hubble Space Telescope.

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Journal
Physical review. D/Physical review. D.
Published
2024-10-03
DOI
https://doi.org/10.1103/physrevd.110.083510
Citations
57
Primary Topic
Galaxies: Formation, Evolution, Phenomena
Type
article
Field-Weighted Citation Impact
18.90

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article

SPT clusters with DES and HST weak lensing. II. Cosmological constraints from the abundance of massive halos

Matthew Young, A. Roodman, C. Romero, N. W. Halverson et al.
57 citations
Physical review. D/Physical review. D.
Galaxies: Formation, Evolution, Phenomena
18.90
article

SPT clusters with DES and HST weak lensing. II. Cosmological constraints from the abundance of massive halos

Matthew Young, A. Roodman, C. Romero, N. W. Halverson, K. Herner, S. S. Meyer, I. Ferrero, P. Chaubal, S. R. Hinton, V. Novosad, B. Yin, I. Harrison, J. García-Bellido, S. Bocquet, S. W. Allen, C. L. Reichardt, J. L. Marshall, F. Kéruzoré, Guillaume Mahler, L. N. da Costa, M. R. Becker, J. E. Carlstrom, R Chen, P. A. R. Ade, D. J. James, K. D. Irwin, C. Davis, J. Frieman, A. J. Anderson, Gourav Khullar, D. Gruen, V. Yefremenko, F. J. Castander, S. Grandis, B. Ansarinejad, P. Paschos, Jason E. Austermann, T. Schrabback, Santiago Avila, A. A. Plazas, Michael D. Gladders, T.-L. Chou, Lincoln Bryant, Gregory Tarlé, D. Sanchez Cid, M. Gatti, B. A. Benson, D. Li, J. Prat, A. Amon, K. Eckert, A. Porredon, J. Myles, M. Brodwin, A Navarro-Alsina, Sahil Pandey, B. Stalder, Eric Huff, T. Natoli, E. M. George, C. Corbett Moran, O. Alves, K. Sharon, L. E. Bleem, V. Strazzullo, G. Giannini, I. Tutusaus, N. MacCrann, G. M. Bernstein, H. Zohren, A. N. Bender, A. Vikhlinin, E. Sheldon, C. Chang, J. E. Ruhl, J. D. Hrubes, Martin W. Sommer, J. Carretero, E. S. Rykoff, C. Tucker, E. Krause, J. Montgomery, N. Weaverdyck, Scott Dodelson, T. M. C. Abbott, T. Shin, J. B. Stephen, J. Elvin-Poole, J. McCullough, Todd Veach, M. Raveri, Y. Omori, S. Everett, A. Mantz, M. Bayliss, N. Gupta, Eusebio Sanchez, J. Weller, B. R. Saliwanchik, J. Mena-Fernández, A. Campos, Ralph Kraft, A. Carnero Rosell, A. T. Crites, C. Sievers, T. N. Varga, J. P. Nibarger, N. Huang, F. Bianchini, K. Kuehn, P.-F. Léget, C. To, L. F. Secco, R. A. Gruendl, W. L. Holzapfel, N. Kuropatkin, J. García-Bellido, F. Menanteau, J. J. Mohr, Taweewat Somboonpanyakul, A. Ferté, Anja von der Linden, Mike Jarvis, G. I. Noble, M. Dobbs, G. Gutierrez, C. Sánchez, J. A. Beall, T. M. Davis, R. L. C. Ogando, A. Choi, Jason Gallicchio, W. Everett, C. L. Chang, A. Alarcon, M. E. S. Pereira, R. P. Rollins, R. Citron, H. T. Diehl, A. T. Lee, Dragan Huterer, A. Pieres, C. Doux, M. Costanzi, A. A. Stark, I. Sevilla-Noarbe, S. Patil, M. McDonald, O. Lahav, J. A. Zebrowski, Johannes Hubmayr, Y Zhang, Matthias Klein, H. C. Chiang, A. E. Lowitz, H. Lin, K. Bechtol, J. Annis, T. de Haan, M. A. Troxel, S Bhargava, L. Salvati, M. Soares-Santos, M. Carrasco Kind, J. J. McMahon, G. P. Holder, Graeme Smecher, R. Miquel, Nathan Whitehorn, W. G. Hartley, J. D. Vieira, A. Drlica-Wagner, K. Honscheid, J. Cordero, A. Saro, C. Pryke, S. Padin, M. Aguena, M. Smith, J. Zuntz, R. Cawthon, D. Bacon, J. DeRose, D. Brooks, B. Yanny, Joseph Roberson, A. M. Flores, K. K. Schaffer, K. Kim, W. L. K. Wu, T. M. Crawford, L. Knox, S. Allam, J. K. Wuko, R. E. A. Canning, S. Desai
article en
57 citations

Abstract

In these two papers, the authors use mock maps to establish a method for studying the abundance and calibrating the weak-lensing based mass of galaxy clusters. They set up a likelihood function, thus obtaining cosmological constraints from a sample of 1,005 clusters detected with the South Pole Telescope, in combination with further cluster data from the Dark Energy Survey, the Wide-field Infrared Survey Explorer, and the Hubble Space Telescope.

Physical review. D/Physical review. D.Vol. 110(8)
Canadian Institute for Advanced Research (CA), University of Geneva (CH), Institució Catalana de Recerca i Estudis Avançats (ES), California Institute of Technology (US), Argonne National Laboratory (US), Oak Ridge National Laboratory (US), Southwest Research Institute (US), Commonwealth Scientific and Industrial Research Organisation (AU), Goddard Space Flight Center (US), Fermi National Accelerator Laboratory (US), National Institute of Standards and Technology (US), Institute of Space Sciences (ES), Harvey Mudd College (US), University of Wisconsin–Madison (US), University of Arizona (US), High Energy Accelerator Research Organization (JP), University of Trieste (IT), Lawrence Berkeley National Laboratory (US), University of Waterloo (CA), University of Illinois Urbana-Champaign (US), Universidad de La Laguna (ES), Chulalongkorn University (TH), Universität Hamburg (DE), Istituto Nazionale di Fisica Nucleare (IT), University of Sussex (GB), The University of Queensland (AU), The University of Melbourne (AU), Duke University (US), Université Fédérale de Toulouse Midi-Pyrénées (FR), Universidade Estadual de Campinas (UNICAMP) (BR), University of Toronto (CA), Durham University (GB), Universität Innsbruck (AT), Brookhaven National Laboratory (US), Princeton University (US), Cornell University (US), University of Cambridge (GB), University of Michigan (US), Lowell Observatory (US), University of Minnesota System (US), Trieste Astronomical Observatory (IT), Mitchell Institute (US), SLAC National Accelerator Laboratory (US), University of Colorado System (US), University of California System (US), University of Manchester (GB), Institute for High Performance Computing and Networking (IT), Lander Institute (IL), California University of Pennsylvania (US), University of Chicago (US), Max Planck Institute for Extraterrestrial Physics (DE), Institut d'Estudis Espacials de Catalunya (ES), Excellence Cluster Origins (DE), Institute of Particle Physics (CA), Centre for Theoretical Physics and Astrophysics (UZ), Center for Astrophysics Harvard & Smithsonian (US), National Observatory (BR), Istituto Nazionale di Fisica Nucleare, Sezione di Genova (IT), Instituto de Astrofísica de Canarias (ES), Barcelona Institute of Science and Technology (ES), Institute for Physics (US), Three-Speed Logic (Canada) (CA), Laboratoire de Physique Subatomique et de Cosmologie (FR), NSF NOIRLab (US), Astronomy and Space (AU), Laboratório Interinstitucional de e-Astronomia (BR), Institute for Fundamental Physics of the Universe (IT), Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas (ES), University of Southampton (GB), Institute of Science and Technology, Institut des langues et cultures d'Europe, Amérique, Afrique, Asie et Australie (FR), University College London (GB), McGill University (CA), The Ohio State University (US), Case Western Reserve University (US), Stony Brook University (US), William Jewell College (US), University of Portsmouth (GB), University of Cincinnati (US), Universidad Autónoma de Madrid (ES), Massachusetts Institute of Technology (US), Indian Institute of Technology Hyderabad (IN), Carnegie Mellon University (US), University of Missouri (US), Cardiff University (GB), Ludwig-Maximilians-Universität München (DE), Michigan State University (US), Université Grenoble Alpes (FR), Ruhr University Bochum (DE), Texas A&M University (US), University of KwaZulu-Natal (ZA), Stanford University (US), University of Edinburgh (GB), Macquarie University (AU)
National Science Foundation, U.S. Department of Energy, National Aeronautics and Space Administration, Stanford University, University of California, University of Pennsylvania, Ohio State University, University of Michigan, Texas A and M University, University of Portsmouth, National Centre for Supercomputing Applications, Higher Education Funding Council for England, Space Telescope Science Institute, Centres de Recerca de Catalunya, Ministarstvo znanosti i obrazovanja, Bundesministerium für Klimaschutz, Umwelt, Energie, Mobilität, Innovation und Technologie, University of Cambridge, University College London, European Commission, University of Nottingham, University of Sussex, University of Edinburgh, Deutsche Forschungsgemeinschaft, Generalitat de Catalunya, Deutsches Zentrum für Luft- und Raumfahrt, Eidgenössische Technische Hochschule Zürich, Ministerio de Ciencia, Tecnología e Innovación Productiva, Ministério da Ciência, Tecnologia e Inovação, Conselho Nacional de Desenvolvimento Científico e Tecnológico, Korea Astronomy and Space Science Institute, Fundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de Janeiro, Financiadora de Estudos e Projetos, Ministerio de Ciencia e Innovación, Österreichische Forschungsförderungsgesellschaft, Ludwig-Maximilians-Universität München, Bundesministerium für Wirtschaft und Energie, Instituto Nacional de Ciência e Tecnologia: Física Nuclear e Aplicações, Institut de Física d'Altes Energies, University of Illinois at Urbana-Champaign, Office of Science, Kavli Institute for Cosmological Physics, University of Chicago, Science and Technology Facilities Council, European Research Council, Australian Research Council, Comisión Nacional de Investigación Científica y Tecnológica, European Regional Development Fund, Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas, High Energy Physics, Astrophysics Division, Fermilab, Lawrence Berkeley National Laboratory, SLAC National Accelerator Laboratory
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Galaxies: Formation, Evolution, Phenomena
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