SPT clusters with DES and HST weak lensing. I. Cluster lensing and Bayesian population modeling of multiwavelength cluster datasets

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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Publication Details

Journal
Physical review. D/Physical review. D.
Published
2024-10-03
DOI
https://doi.org/10.1103/physrevd.110.083509
Citations
25
Primary Topic
Galaxies: Formation, Evolution, Phenomena
Type
article
Field-Weighted Citation Impact
8.29

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article

SPT clusters with DES and HST weak lensing. I. Cluster lensing and Bayesian population modeling of multiwavelength cluster datasets

A. Roodman, K. Eckert, D. Sanchez Cid, I. Ferrero et al.
25 citations
Physical review. D/Physical review. D.
Galaxies: Formation, Evolution, Phenomena
8.29
article

SPT clusters with DES and HST weak lensing. I. Cluster lensing and Bayesian population modeling of multiwavelength cluster datasets

A. Roodman, K. Eckert, D. Sanchez Cid, I. Ferrero, J. Cordero, S. R. Hinton, J. Myles, S Pandey, D. Brooks, T. N. Varga, J. Carretero, B. Yin, I. Harrison, J. García-Bellido, S. Bocquet, S. Allam, S. W. Allen, C. L. Reichardt, J. L. Marshall, F. Kéruzoré, Guillaume Mahler, L. N. da Costa, N.P. Kuropatkin, M. R. Smith, M. R. Becker, A. Saro, J. E. Carlstrom, C. Romero, Michael S. Schubnell, R Chen, C. Davis, Gourav Khullar, D. Gruen, J. DeRose, S. Grandis, T. Schrabback, Robert P. Kraft, A. A. Plazas, Michael D. Gladders, Keunho Kim, A. K. Romer, Gregory Tarlé, M. Gatti, B. A. Benson, E. Suchyta, J. Prat, E. Sheldon, A. Amon, A Navarro-Alsina, J. Zuntz, O. Alves, K. Sharon, P. Wiseman, L. E. Bleem, V. Strazzullo, G. Giannini, I. Tutusaus, N. MacCrann, G. M. Bernstein, C. Chang, E. S. Rykoff, N. Weaverdyck, D. J. James, Scott Dodelson, A. Palmese, T. Shin, J. Elvin-Poole, J. McCullough, M. Raveri, S. Everett, K. Bechtol, A. Mantz, M. Bayliss, Eusebio Sanchez, J. Weller, J. Mena-Fernández, A. Campos, Ashley J. Ross, A. Carnero Rosell, Behzad Ansarinejad, K. Kuehn, B. Stalder, P.-F. Léget, C. To, R. A. Gruendl, W. L. Holzapfel, J. García-Bellido, J. J. Mohr, David Bacon, Taweewat Somboonpanyakul, A. Ferté, Anja von der Linden, Mike Jarvis, C. Sánchez, S. Lee, R. L. C. Ogando, K. Herner, A. Choi, R. Miquel, Y. Zhang, A. Alarcon, M. E. S. Pereira, R. P. Rollins, H. T. Diehl, S. Desai, C. Doux, R. Cawthon, M. Aguena, M. Costanzi, A. A. Stark, I. Sevilla-Noarbe, M. McDonald, Matthias Klein, Rebecca Canning, T. de Haan, M. A. Troxel, L. Salvati, P. Doel, M. Carrasco Kind, Joshua A. Frieman, M. E. C. Swanson, W. G. Hartley, M. R. Young, L F Secco, A. Drlica-Wagner, K. Honscheid, A. Pieres, M. Brodwin, E. M. Huff, N. Huang, B. Yanny, Joseph Roberson, A. M. Flores, J. De Vicente
article en
25 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)
University of Geneva (CH), Institució Catalana de Recerca i Estudis Avançats (ES), California Institute of Technology (US), Argonne National Laboratory (US), Goddard Space Flight Center (US), Fermi National Accelerator Laboratory (US), University of Wisconsin–Madison (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), University of Cambridge (GB), Université Paris-Saclay (FR), University of Michigan (US), Lowell Observatory (US), Geophysical Survey (RU), Trieste Astronomical Observatory (IT), Mitchell Institute (US), SLAC National Accelerator Laboratory (US), Brera Astronomical Observatory (IT), 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), Excellence Cluster Origins (DE), Institute of Particle Physics (CA), Centre for Theoretical Physics and Astrophysics (UZ), Center for Astrophysics Harvard & Smithsonian (US), 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), NSF NOIRLab (US), 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), The Ohio State 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), Université Grenoble Alpes (FR), Texas A&M University (US), Stanford University (US), University of Edinburgh (GB), Macquarie University (AU)
National Science Foundation, U.S. Department of Energy, Stanford University, University of California, University of Pennsylvania, Ohio State University, University of Chicago, University of Michigan, Texas A and M University, University of Portsmouth, Bundesministerium für Klimaschutz, Umwelt, Energie, Mobilität, Innovation und Technologie, University of Cambridge, University College London, University of Nottingham, University of Sussex, University of Edinburgh, Deutsche Forschungsgemeinschaft, Generalitat de Catalunya, Deutsches Zentrum für Luft- und Raumfahrt, Eidgenössische Technische Hochschule Zürich, Ministério da Ciência, Tecnologia e Inovação, Conselho Nacional de Desenvolvimento Científico e Tecnológico, Max-Planck-Gesellschaft, 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, Ministerio de Ciencia y Tecnología, 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, European Regional Development Fund, Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas, High Energy Physics, Argonne National Laboratory, Fermilab, Lawrence Berkeley National Laboratory, SLAC National Accelerator Laboratory
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Galaxies: Formation, Evolution, Phenomena
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