Euclid preparation. XLII. A unified catalogue-level reanalysis of weak lensing by galaxy clusters in five imaging surveys
Euclid Collaboration, M. Sereno (INAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Bologna, Italy, INFN-Sezione di Bologna, Bologna, Italy), S. Farrens (Universit’e Paris-Saclay, Universit’e Paris Cit’e, CEA, CNRS, AIM, Gif-sur-Yvette, France), L. Ingoglia (Dipartimento di Fisica e Astronomia "Augusto Righi" – Alma Mater Studiorum Universit`a di Bologna, Bologna, Italy), G. F. Lesci (Dipartimento di Fisica e Astronomia "Augusto Righi" – Alma Mater Studiorum Universit`a di Bologna, Bologna, Italy, INAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Bologna, Italy), L. Baumont (AIM, CEA, CNRS, Universit’e Paris-Saclay, Universit’e de Paris, Gif-sur-Yvette, France), G. Covone (Department of Physics "E. Pancini", University Federico II, Napoli, Italy, INAF-Osservatorio Astronomico di Capodimonte, Napoli, Italy, INFN section of Naples, Napoli, Italy), C. Giocoli (INAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Bologna, Italy, INFN-Sezione di Bologna, Bologna, Italy), F. Marulli (Dipartimento di Fisica e Astronomia "Augusto Righi" – Alma Mater Studiorum Universit`a di Bologna, Bologna, Italy, INAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Bologna, Italy, INFN-Sezione di Bologna, Bologna, Italy), S. Miranda La Hera (Universit’e Paris-Saclay, Universit’e Paris Cit’e, CEA, CNRS, AIM, Gif-sur-Yvette, France), M. Vannier (Universit’e C^ote d’Azur, Observatoire de la C^ote d’Azur, CNRS, Laboratoire Lagrange, Bd de l’Observatoire, CS 34229, Nice, France), A. Biviano (INAF-Osservatorio Astronomico di Trieste, Trieste, Italy, IFPU, Institute for Fundamental Physics of the Universe, Trieste, Italy), S. Maurogordato (Universit’e C^ote d’Azur, Observatoire de la C^ote d’Azur, CNRS, Laboratoire Lagrange, Bd de l’Observatoire, CS 34229, Nice, France), L. Moscardini (Dipartimento di Fisica e Astronomia "Augusto Righi" – Alma Mater Studiorum Universit`a di Bologna, Bologna, Italy, INAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Bologna, Italy, INFN-Sezione di Bologna, Bologna, Italy), N. Aghanim (Universit’e Paris-Saclay, CNRS, Institut d’astrophysique spatiale, Orsay, France), S. Andreon (INAF-Osservatorio Astronomico di Brera, Milano, Italy), N. Auricchio (INAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Bologna, Italy), M. Baldi (Dipartimento di Fisica e Astronomia "Augusto Righi" – Alma Mater Studiorum Universit`a di Bologna, Bologna, Italy, INAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Bologna, Italy, INFN-Sezione di Bologna, Bologna, Italy), S. Bardelli (INAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Bologna, Italy), F. Bellagamba (Dipartimento di Fisica e Astronomia, Universit`a di Bologna, Bologna, Italy, INAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Bologna, Italy), C. Bodendorf (Max Planck Institute for Extraterrestrial Physics, Garching, Germany), D. Bonino (INAF-Osservatorio Astrofisico di Torino, Pino Torinese), E. Branchini (Dipartimento di Fisica, Universit`a di Genova, Genova, Italy, INFN-Sezione di Genova, Genova, Italy), M. Brescia (Department of Physics "E. Pancini", University Federico II, Napoli, Italy, INAF-Osservatorio Astronomico di Capodimonte, Napoli, Italy), J. Brinchmann (Instituto de Astrof’isica e Ci^encias do Espac{c}o, Universidade do Porto, CAUP, Porto, Portugal), S. Camera (Dipartimento di Fisica, Universit`a degli Studi di Torino, Torino, Italy, INFN-Sezione di Torino, Torino, Italy, INAF-Osservatorio Astrofisico di Torino, Pino Torinese), V. Capobianco (INAF-Osservatorio Astrofisico di Torino, Pino Torinese), C. Carbone (INAF-IASF Milano, Milano, Italy), V. F. Cardone (INAF-Osservatorio Astronomico di Roma, Monteporzio Catone, Italy, INFN-Sezione di Roma, Piazzale Aldo Moro, 2 – c/o Dipartimento di Fisica, Edificio G. Marconi, Roma, Italy), J. Carretero (Institut de F’isica d’Altes Energies, Port d’Informaci’o Cient’ifica, Campus UAB, C. Albareda s/n, Barcelona, Spain), S. Casas (Institute for Theoretical Particle Physics and Cosmology), M. Castellano (INAF-Osservatorio Astronomico di Roma, Monteporzio Catone, Italy), S. Cavuoti (INAF-Osservatorio Astronomico di Capodimonte, Napoli, Italy, INFN section of Naples, Napoli, Italy), A. Cimatti (Dipartimento di Fisica e Astronomia "Augusto Righi" – Alma Mater Studiorum Universit`a di Bologna, Bologna, Italy), R. Cledassou (Centre National d’Etudes Spatiales — Centre spatial de Toulouse, Toulouse, France, Institut national de physique nucl’eaire et de physique des particules, Paris, France), G. Congedo (Institute for Astronomy, University of Edinburgh, Royal Observatory, Edinburgh, UK), C. J. Conselice (Jodrell Bank Centre for Astrophysics, Department of Physics and Astronomy, University of Manchester, Manchester, UK), L. Conversi (European Space Agency/ESRIN, Largo Galileo Galilei 1, Roma, Italy, ESAC/ESA, Camino Bajo del Castillo, s/n., Urb. Villafranca del Castillo, Madrid, Spain), Y. Copin (Universit’e Claude Bernard Lyon 1, CNRS/IN2P3, IP2I Lyon, Villeurbanne, France), L. Corcione (INAF-Osservatorio Astrofisico di Torino, Pino Torinese), F. Courbin (Institute of Physics, Laboratory of Astrophysics, Ecole Polytechnique F’ed’erale de Lausanne), H. M. Courtois (UCB Lyon 1, CNRS/IN2P3, IUF, IP2I Lyon, Villeurbanne, France), M. Cropper (Mullard Space Science Laboratory, University College London, Holmbury St Mary, Dorking, Surrey, UK), A. Da Silva (Departamento de F’isica, Faculdade de Ci^encias, Universidade de Lisboa, Edif’icio C8, Lisboa, Portugal, Instituto de Astrof’isica e Ci^encias do Espac{c}o, Faculdade de Ci^encias, Universidade de Lisboa, Lisboa, Portugal), H. Degaudenzi (Department of Astronomy, University of Geneva, Versoix, Switzerland), A. M. Di Giorgio (INAF-Istituto di Astrofisica e Planetologia Spaziali, Roma, Italy), J. Dinis (Instituto de Astrof’isica e Ci^encias do Espac{c}o, Faculdade de Ci^encias, Universidade de Lisboa, Lisboa, Portugal, Departamento de F’isica, Faculdade de Ci^encias, Universidade de Lisboa, Edif’icio C8, Lisboa, Portugal), F. Dubath (Department of Astronomy, University of Geneva, Versoix, Switzerland), C. A. J. Duncan (Department of Physics, Oxford University, Oxford, UK, Jodrell Bank Centre for Astrophysics, Department of Physics and Astronomy, University of Manchester, Manchester, UK), X. Dupac (ESAC/ESA, Camino Bajo del Castillo, s/n., Urb. Villafranca del Castillo, Madrid, Spain), S. Dusini (INFN-Padova, Padova, Italy), M. Farina (INAF-Istituto di Astrofisica e Planetologia Spaziali, Roma, Italy), S. Ferriol (Universit’e Claude Bernard Lyon 1, CNRS/IN2P3, IP2I Lyon, Villeurbanne, France), M. Frailis (INAF-Osservatorio Astronomico di Trieste, Trieste, Italy), E. Franceschi (INAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Bologna, Italy), M. Fumana (INAF-IASF Milano, Milano, Italy), S. Galeotta (INAF-Osservatorio Astronomico di Trieste, Trieste, Italy), B. Garilli (INAF-IASF Milano, Milano, Italy), B. Gillis (Institute for Astronomy, University of Edinburgh, Royal Observatory, Edinburgh, UK), A. Grazian (INAF-Osservatorio Astronomico di Padova, Padova, Italy), F. Grupp (Max Planck Institute for Extraterrestrial Physics, Garching, Germany, Universit"ats-Sternwarte M"unchen, Fakult"at f"ur Physik, Ludwig-Maximilians-Universit"at M"unchen, M"unchen, Germany), S. V. H. Haugan (Institute of Theoretical Astrophysics, University of Oslo, Oslo, Norway), W. Holmes (Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, USA), I. Hook (Department of Physics, Lancaster University, Lancaster, UK), F. Hormuth (von Hoerner & Sulger GmbH, Schwetzingen, Germany), A. Hornstrup (Technical University of Denmark, Lyngby, Denmark, Cosmic Dawn Center), P. Hudelot (Institut d’Astrophysique de Paris, UMR 7095, CNRS, and Sorbonne Universit’e, Paris, France), K. Jahnke (Max-Planck-Institut f"ur Astronomie, Heidelberg, Germany), B. Joachimi (Department of Physics and Astronomy, University College London, London, UK), E. Keih"anen (Department of Physics and Helsinki Institute of Physics, University of Helsinki, Finland), S. Kermiche (Aix-Marseille Universit’e, Marseille, France), A. Kiessling (Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, USA), B. Kubik (Universit’e Claude Bernard Lyon 1, CNRS/IN2P3, IP2I Lyon, Villeurbanne, France), M. Kunz (Universit’e de Gen`eve, D’epartement de Physique Th’eorique and Centre for Astroparticle Physics, Gen`eve, Switzerland), H. Kurki-Suonio (Department of Physics, University of Helsinki, Finland, Helsinki Institute of Physics, Gustaf H"allstr"omin katu 2, University of Helsinki, Helsinki, Finland), S. Ligori (INAF-Osservatorio Astrofisico di Torino, Pino Torinese), P. B. Lilje (Institute of Theoretical Astrophysics, University of Oslo, Oslo, Norway), V. Lindholm (Department of Physics, University of Helsinki, Finland, Helsinki Institute of Physics, Gustaf H"allstr"omin katu 2, University of Helsinki, Helsinki, Finland), I. Lloro (NOVA optical infrared instrumentation group at ASTRON, Dwingeloo, The Netherlands), D. Maino (Dipartimento di Fisica "Aldo Pontremoli", Universit`a degli Studi di Milano, Milano, Italy, INAF-IASF Milano, Milano, Italy, INFN-Sezione di Milano, Milano, Italy), E. Maiorano (INAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Bologna, Italy), O. Mansutti (INAF-Osservatorio Astronomico di Trieste, Trieste, Italy), O. Marggraf (Universit"at Bonn, Argelander-Institut f"ur Astronomie, Bonn, Germany), K. Markovic (Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, USA), N. Martinet (Aix-Marseille Universit’e, CNRS, CNES, LAM, Marseille, France), R. Massey (Department of Physics, Institute for Computational Cosmology, Durham University, South Road, UK), E. Medinaceli (INAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Bologna, Italy), S. Mei (Universit’e Paris Cit’e, CNRS, Astroparticule et Cosmologie, Paris, France), Y. Mellier (Institut d’Astrophysique de Paris, Paris, France, Institut d’Astrophysique de Paris, UMR 7095, CNRS, and Sorbonne Universit’e, Paris, France), M. Meneghetti (INAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Bologna, Italy, INFN-Sezione di Bologna, Bologna, Italy), E. Merlin (INAF-Osservatorio Astronomico di Roma, Monteporzio Catone, Italy), G. Meylan (Institute of Physics, Laboratory of Astrophysics, Ecole Polytechnique F’ed’erale de Lausanne), M. Moresco (Dipartimento di Fisica e Astronomia "Augusto Righi" – Alma Mater Studiorum Universit`a di Bologna, Bologna, Italy, INAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Bologna, Italy), E. Munari (INAF-Osservatorio Astronomico di Trieste, Trieste, Italy), S. -M. Niemi (European Space Agency/ESTEC, The Netherlands), T. Nutma (Kapteyn Astronomical Institute, University of Groningen, Groningen, The Netherlands, Leiden Observatory, Leiden University, CC Leiden, The Netherlands), C. Padilla (Institut de F’isica d’Altes Energies), S. Paltani (Department of Astronomy, University of Geneva, Versoix, Switzerland), F. Pasian (INAF-Osservatorio Astronomico di Trieste, Trieste, Italy), K. Pedersen (Department of Physics and Astronomy, University of Aarhus, Aarhus C, Denmark), V. Pettorino (Universit’e Paris-Saclay, Universit’e Paris Cit’e, CEA, CNRS, Astrophysique, Instrumentation et Mod’elisation Paris-Saclay, Gif-sur-Yvette, France), S. Pires (Universit’e Paris-Saclay, Universit’e Paris Cit’e, CEA, CNRS, AIM, Gif-sur-Yvette, France), G. Polenta (Space Science Data Center, Italian Space Agency, via del Politecnico snc, Roma, Italy), M. Poncet (Centre National d’Etudes Spatiales — Centre spatial de Toulouse, Toulouse, France), L. A. Popa (Institute of Space Science, Str. Atomistilor, Ilfov, Romania), F. Raison (Max Planck Institute for Extraterrestrial Physics, Garching, Germany), R. Rebolo (Instituto de Astrof’isica de Canarias, San Crist’obal de La Laguna, Tenerife, Spain, Departamento de Astrof’isica, Universidad de La Laguna, La Laguna, Tenerife, Spain), A. Renzi (Dipartimento di Fisica e Astronomia "G. Galilei", Universit`a di Padova, Padova, Italy, INFN-Padova, Padova, Italy), J. Rhodes (Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, USA), G. Riccio (INAF-Osservatorio Astronomico di Capodimonte, Napoli, Italy), E. Romelli (INAF-Osservatorio Astronomico di Trieste, Trieste, Italy), M. Roncarelli (INAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Bologna, Italy), E. Rossetti (Dipartimento di Fisica e Astronomia, Universit`a di Bologna, Bologna, Italy), R. Saglia (Universit"ats-Sternwarte M"unchen, Fakult"at f"ur Physik, Ludwig-Maximilians-Universit"at M"unchen, M"unchen, Germany, Max Planck Institute for Extraterrestrial Physics, Garching, Germany), D. Sapone (Departamento de F’isica, FCFM, Universidad de Chile, Santiago, Chile), B. Sartoris (Universit"ats-Sternwarte M"unchen, Fakult"at f"ur Physik, Ludwig-Maximilians-Universit"at M"unchen, M"unchen, Germany, INAF-Osservatorio Astronomico di Trieste, Trieste, Italy), M. Schirmer (Max-Planck-Institut f"ur Astronomie, Heidelberg, Germany), P. Schneider (Universit"at Bonn, Argelander-Institut f"ur Astronomie, Bonn, Germany), T. Schrabback (Universit"at Innsbruck, Institut f"ur Astro- und Teilchenphysik, Austria), A. Secroun (Aix-Marseille Universit’e, Marseille, France), G. Seidel (Max-Planck-Institut f"ur Astronomie, Heidelberg, Germany), S. Serrano (Institut d’Estudis Espacials de Catalunya, Institut de Ciencies de l’Espai), C. Sirignano (Dipartimento di Fisica e Astronomia "G. Galilei", Universit`a di Padova, Padova, Italy, INFN-Padova, Padova, Italy), G. Sirri (INFN-Sezione di Bologna, Bologna, Italy), L. Stanco (INFN-Padova, Padova, Italy), J. -L. Starck (AIM, CEA, CNRS, Universit’e Paris-Saclay, Universit’e de Paris, Gif-sur-Yvette, France), P. Tallada-Cresp’i (Centro de Investigaciones Energ’eticas, Medioambientales y Tecnol’ogicas, Port d’Informaci’o Cient’ifica, Campus UAB, C. Albareda s/n, Barcelona, Spain), A. N. Taylor (Institute for Astronomy, University of Edinburgh, Royal Observatory, Edinburgh, UK), I. Tereno (Departamento de F’isica, Faculdade de Ci^encias, Universidade de Lisboa, Edif’icio C8, Lisboa, Portugal, Instituto de Astrof’isica e Ci^encias do Espac{c}o, Faculdade de Ci^encias, Universidade de Lisboa, Lisboa, Portugal), R. Toledo-Moreo (Universidad Polit’ecnica de Cartagena, Departamento de Electr’onica y Tecnolog’ia de Computadoras, Cartagena, Spain), F. Torradeflot (Port d’Informaci’o Cient’ifica, Campus UAB, C. Albareda s/n, Barcelona, Spain, Centro de Investigaciones Energ’eticas, Medioambientales y Tecnol’ogicas), I. Tutusaus (Institut de Recherche en Astrophysique et Plan’etologie), E. A. Valentijn (Kapteyn Astronomical Institute, University of Groningen, Groningen, The Netherlands), L. Valenziano (INAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Bologna, Italy, INFN-Bologna, Bologna, Italy), T. Vassallo (INAF-Osservatorio Astronomico di Trieste, Trieste, Italy, Universit"ats-Sternwarte M"unchen, Fakult"at f"ur Physik, Ludwig-Maximilians-Universit"at M"unchen, M"unchen, Germany), A. Veropalumbo (INAF-Osservatorio Astronomico di Brera, Milano, Italy), Y. Wang (Infrared Processing and Analysis Center, California Institute of Technology, Pasadena, CA, USA), J. Weller (Universit"ats-Sternwarte M"unchen, Fakult"at f"ur Physik, Ludwig-Maximilians-Universit"at M"unchen, M"unchen, Germany, Max Planck Institute for Extraterrestrial Physics, Garching, Germany), A. Zacchei (INAF-Osservatorio Astronomico di Trieste, Trieste, Italy, IFPU, Institute for Fundamental Physics of the Universe, Trieste, Italy), G. Zamorani (INAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Bologna, Italy), J. Zoubian (Aix-Marseille Universit’e, Marseille, France), E. Zucca (INAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Bologna, Italy), A. Boucaud (Universit’e Paris Cit’e, CNRS, Astroparticule et Cosmologie, Paris, France), E. Bozzo (Department of Astronomy, University of Geneva, Versoix, Switzerland), C. Cerna (Institut d’Astrophysique de Paris, UMR 7095, CNRS, and Sorbonne Universit’e, Paris, France, CEA Saclay, DFR/IRFU, Service d’Astrophysique, Gif-sur-Yvette, France), C. Colodro-Conde (Instituto de Astrof’isica de Canarias, San Crist’obal de La Laguna, Tenerife, Spain), D. Di Ferdinando (INFN-Sezione di Bologna, Bologna, Italy), R. Farinelli (INAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Bologna, Italy), H. Israel (Ernst-Reuter-Str. 4e, Peine, Germany), N. Mauri (Dipartimento di Fisica e Astronomia "Augusto Righi" – Alma Mater Studiorum Universit`a di Bologna, Bologna, Italy, INFN-Sezione di Bologna, Bologna, Italy), C. Neissner (Institut de F’isica d’Altes Energies, Port d’Informaci’o Cient’ifica, Campus UAB, C. Albareda s/n, Barcelona, Spain), V. Scottez (Institut d’Astrophysique de Paris, Paris, France, Junia, EPA department, Lille, France), M. Tenti (INFN-Bologna, Bologna, Italy), M. Wiesmann (Institute of Theoretical Astrophysics, University of Oslo, Oslo, Norway), Y. Akrami (Instituto de F’isica Te’orica UAM-CSIC, Campus de Cantoblanco, Madrid, Spain, CERCA/ISO, Department of Physics, Case Western Reserve University, Cleveland, OH, USA, Laboratoire de Physique de l”Ecole Normale Sup’erieure, ENS, Universit’e PSL, CNRS, Sorbonne Universit’e, Paris, France, Observatoire de Paris, Universit’e PSL, Sorbonne Universit’e, LERMA, Paris, France, Astrophysics Group, Blackett Laboratory, Imperial College London, London, UK), V. Allevato (INAF-Osservatorio Astronomico di Capodimonte, Napoli, Italy, Scuola Normale Superiore, Pisa, Italy), C. Baccigalupi (SISSA, International School for Advanced Studies, Trieste TS, Italy, IFPU, Institute for Fundamental Physics of the Universe, Trieste, Italy, INAF-Osservatorio Astronomico di Trieste, Trieste, Italy, INFN, Sezione di Trieste, Trieste TS, Italy), M. Ballardini (Dipartimento di Fisica e Scienze della Terra, Universit`a degli Studi di Ferrara, Ferrara, Italy, Istituto Nazionale di Fisica Nucleare, Sezione di Ferrara, Ferrara, Italy, INAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Bologna, Italy), D. Benielli (Aix-Marseille Universit’e, Marseille, France), S. Borgani (INAF-Osservatorio Astronomico di Trieste, Trieste, Italy, Dipartimento di Fisica – Sezione di Astronomia, Universit`a di Trieste, Trieste, Italy, INFN, Sezione di Trieste, Trieste TS, Italy, IFPU, Institute for Fundamental Physics of the Universe, Trieste, Italy), A. S. Borlaff (NASA Ames Research Center, Moffett Field, CA, USA, Kavli Institute for Particle Astrophysics & Cosmology), C. Burigana (INAF, Istituto di Radioastronomia, Bologna, Italy, INFN-Bologna, Bologna, Italy), R. Cabanac (Institut de Recherche en Astrophysique et Plan’etologie), A. Cappi (INAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Bologna, Italy, Universit’e C^ote d’Azur, Observatoire de la C^ote d’Azur, CNRS, Laboratoire Lagrange, Bd de l’Observatoire, CS 34229, Nice, France), C. S. Carvalho (Instituto de Astrof’isica e Ci^encias do Espac{c}o, Faculdade de Ci^encias, Universidade de Lisboa, Lisboa, Portugal), G. Castignani (Dipartimento di Fisica e Astronomia "Augusto Righi" – Alma Mater Studiorum Universit`a di Bologna, Bologna, Italy, INAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Bologna, Italy), T. Castro (INAF-Osservatorio Astronomico di Trieste, Trieste, Italy, INFN, Sezione di Trieste, Trieste TS, Italy, IFPU, Institute for Fundamental Physics of the Universe, Trieste, Italy), G. Ca~nas-Herrera (European Space Agency/ESTEC, The Netherlands, Institute Lorentz, Leiden University, Leiden, The Netherlands), K. C. Chambers (Institute for Astronomy, University of Hawaii, Honolulu, HI, USA), A. R. Cooray (Department of Physics & Astronomy, University of California Irvine, Irvine CA, USA), J. Coupon (Department of Astronomy, University of Geneva, Versoix, Switzerland), S. Davini (INFN-Sezione di Genova, Genova, Italy), G. De Lucia (INAF-Osservatorio Astronomico di Trieste, Trieste, Italy), G. Desprez (Department of Astronomy & Physics and Institute for Computational Astrophysics, Saint Mary’s University, Halifax, Nova Scotia, Canada), S. Di Domizio (Dipartimento di Fisica, Universit`a degli studi di Genova, and INFN-Sezione di Genova, Genova, Italy), H. Dole (Universit’e Paris-Saclay, CNRS, Institut d’astrophysique spatiale, Orsay, France), J. A. Escartin Vigo (Max Planck Institute for Extraterrestrial Physics, Garching, Germany), S. Escoffier (Aix-Marseille Universit’e, Marseille, France), I. Ferrero (Institute of Theoretical Astrophysics, University of Oslo, Oslo, Norway), L. Gabarra (Dipartimento di Fisica e Astronomia "G. Galilei", Universit`a di Padova, Padova, Italy, INFN-Padova, Padova, Italy), E. Gaztanaga (Institute of Space Sciences, Institut d’Estudis Espacials de Catalunya, Institute of Cosmology and Gravitation, University of Portsmouth, Portsmouth, UK), K. George (Universit"ats-Sternwarte M"unchen, Fakult"at f"ur Physik, Ludwig-Maximilians-Universit"at M"unchen, M"unchen, Germany), F. Giacomini (INFN-Sezione di Bologna, Bologna, Italy), G. Gozaliasl (Department of Physics, University of Helsinki, Finland), H. Hildebrandt (Ruhr University Bochum, Faculty of Physics and Astronomy, Astronomical Institute), J. J. E. Kajava (Department of Physics and Astronomy, University of Turku, Finland), V. Kansal (AIM, CEA, CNRS, Universit’e Paris-Saclay, Universit’e de Paris, Gif-sur-Yvette, France), C. C. Kirkpatrick (Department of Physics and Helsinki Institute of Physics, University of Helsinki, Finland), L. Legrand (Universit’e de Gen`eve, D’epartement de Physique Th’eorique and Centre for Astroparticle Physics, Gen`eve, Switzerland), P. Liebing (Mullard Space Science Laboratory, University College London, Holmbury St Mary, Dorking, Surrey, UK), A. Loureiro (Oskar Klein Centre for Cosmoparticle Physics, Department of Physics, Stockholm University, Stockholm, Sweden, Astrophysics Group, Blackett Laboratory, Imperial College London, London, UK), J. Macias-Perez (Univ. Grenoble Alpes, CNRS, Grenoble INP, Grenoble, France), M. Magliocchetti (INAF-Istituto di Astrofisica e Planetologia Spaziali, Roma, Italy), G. Mainetti (Centre de Calcul de l’IN2P3/CNRS, Villeurbanne, France), R. Maoli (Dipartimento di Fisica, Sapienza Universit`a di Roma, Roma, Italy, INAF-Osservatorio Astronomico di Roma, Monteporzio Catone, Italy), M. Martinelli (INAF-Osservatorio Astronomico di Roma, Monteporzio Catone, Italy, INFN-Sezione di Roma, Piazzale Aldo Moro, 2 – c/o Dipartimento di Fisica, Edificio G. Marconi, Roma, Italy), C. J. A. P. Martins (Centro de Astrof’isica da Universidade do Porto, Porto, Portugal, Instituto de Astrof’isica e Ci^encias do Espac{c}o, Universidade do Porto, CAUP, Porto, Portugal), S. Z. Matthew (Institute for Astronomy, University of Edinburgh, Royal Observatory, Edinburgh, UK), M. Maturi (Institut f"ur Theoretische Physik, University of Heidelberg, Heidelberg, Germany, Zentrum f"ur Astronomie, Universit"at Heidelberg, Heidelberg, Germany), L. Maurin (Universit’e Paris-Saclay, CNRS, Institut d’astrophysique spatiale, Orsay, France), R. B. Metcalf (Dipartimento di Fisica e Astronomia "Augusto Righi" – Alma Mater Studiorum Universit`a di Bologna, Bologna, Italy), P. Monaco (Dipartimento di Fisica – Sezione di Astronomia, Universit`a di Trieste, Trieste, Italy, INAF-Osservatorio Astronomico di Trieste, Trieste, Italy, INFN, Sezione di Trieste, Trieste TS, Italy, IFPU, Institute for Fundamental Physics of the Universe, Trieste, Italy), G. Morgante (INAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Bologna, Italy), S. Nadathur (Institute of Cosmology and Gravitation, University of Portsmouth, Portsmouth, UK), A. A. Nucita (Department of Mathematics and Physics E. De Giorgi, University of Salento, Lecce, Italy, INAF-Sezione di Lecce, c/o Dipartimento Matematica e Fisica, Lecce, Italy, INFN, Sezione di Lecce, Lecce, Italy), L. Patrizii (INFN-Sezione di Bologna, Bologna, Italy), A. Peel (Institute of Physics, Laboratory of Astrophysics, Ecole Polytechnique F’ed’erale de Lausanne), M. P"ontinen (Department of Physics, University of Helsinki, Finland), V. Popa (Institute of Space Science, Str. Atomistilor, Ilfov, Romania), C. Porciani (Universit"at Bonn, Argelander-Institut f"ur Astronomie, Bonn, Germany), D. Potter (Department of Astrophysics, University of Zurich, Switzerland), P. Reimberg (Institut d’Astrophysique de Paris, Paris, France), Z. Sakr (Institut de Recherche en Astrophysique et Plan’etologie, Universit’e St Joseph, Faculty of Sciences, Beirut, Lebanon, Institut f"ur Theoretische Physik, University of Heidelberg, Heidelberg, Germany), A. G. S’anchez (Max Planck Institute for Extraterrestrial Physics, Garching, Germany), A. Schneider (Department of Astrophysics, University of Zurich, Switzerland), E. Sefusatti (INAF-Osservatorio Astronomico di Trieste, Trieste, Italy, IFPU, Institute for Fundamental Physics of the Universe, Trieste, Italy, INFN, Sezione di Trieste, Trieste TS, Italy), P. Simon (Universit"at Bonn, Argelander-Institut f"ur Astronomie, Bonn, Germany), A. Spurio Mancini (Mullard Space Science Laboratory, University College London, Holmbury St Mary, Dorking, Surrey, UK), J. Stadel (Department of Astrophysics, University of Zurich, Switzerland), S. A. Stanford (Department of Physics and Astronomy, University of California, Davis, CA, USA), J. Steinwagner (Max Planck Institute for Extraterrestrial Physics, Garching, Germany), R. Teyssier (Department of Astrophysical Sciences, Peyton Hall, Princeton University, Princeton, NJ, USA), J. Valiviita (Department of Physics, University of Helsinki, Finland, Helsinki Institute of Physics, Gustaf H"allstr"omin katu 2, University of Helsinki, Helsinki, Finland), M. Viel (SISSA, International School for Advanced Studies, Trieste TS, Italy, IFPU, Institute for Fundamental Physics of the Universe, Trieste, Italy, INAF-Osservatorio Astronomico di Trieste, Trieste, Italy, INFN, Sezione di Trieste, Trieste TS, Italy)
arXiv:2404.08036v1 Announce Type: new
Abstract: Precise and accurate mass calibration is required to exploit galaxy clusters as astrophysical and cosmological probes in the Euclid era. Systematic errors in lensing signals by galaxy clusters can be empirically estimated by comparing different surveys with independent and uncorrelated systematics. To assess the robustness of the lensing results to systematic errors, we carried out end-to-end tests across different data sets. We performed a unified analysis at the catalogue level by leveraging the Euclid combined cluster and weak-lensing pipeline (COMB-CL). COMB-CL will measure weak lensing cluster masses for the Euclid Survey. Heterogeneous data sets from five independent, recent, lensing surveys (CHFTLenS, DES~SV1, HSC-SSP~S16a, KiDS~DR4, and RCSLenS), which exploited different shear and photometric redshift estimation algorithms, were analysed with a consistent pipeline under the same model assumptions. We performed a comparison of the amplitude of the reduced excess surface density and of the mass estimates using lenses from the Planck PSZ2 and SDSS redMaPPer cluster samples. Mass estimates agree with literature results collected in the LC2 catalogues. Mass accuracy was further investigated considering the AMICO detected clusters in the HSC-SSP XXL North field. The consistency of the data sets was tested using our unified analysis framework. We found agreement between independent surveys, at the level of systematic noise in Stage-III surveys or precursors. This indicates successful control over systematics. If such control continues in Stage-IV, Euclid will be able to measure the weak lensing masses of around 13000 (considering shot noise only) or 3000 (noise from shape and large-scale-structure) massive clusters with a signal-to-noise ratio greater than 3.arXiv:2404.08036v1 Announce Type: new
Abstract: Precise and accurate mass calibration is required to exploit galaxy clusters as astrophysical and cosmological probes in the Euclid era. Systematic errors in lensing signals by galaxy clusters can be empirically estimated by comparing different surveys with independent and uncorrelated systematics. To assess the robustness of the lensing results to systematic errors, we carried out end-to-end tests across different data sets. We performed a unified analysis at the catalogue level by leveraging the Euclid combined cluster and weak-lensing pipeline (COMB-CL). COMB-CL will measure weak lensing cluster masses for the Euclid Survey. Heterogeneous data sets from five independent, recent, lensing surveys (CHFTLenS, DES~SV1, HSC-SSP~S16a, KiDS~DR4, and RCSLenS), which exploited different shear and photometric redshift estimation algorithms, were analysed with a consistent pipeline under the same model assumptions. We performed a comparison of the amplitude of the reduced excess surface density and of the mass estimates using lenses from the Planck PSZ2 and SDSS redMaPPer cluster samples. Mass estimates agree with literature results collected in the LC2 catalogues. Mass accuracy was further investigated considering the AMICO detected clusters in the HSC-SSP XXL North field. The consistency of the data sets was tested using our unified analysis framework. We found agreement between independent surveys, at the level of systematic noise in Stage-III surveys or precursors. This indicates successful control over systematics. If such control continues in Stage-IV, Euclid will be able to measure the weak lensing masses of around 13000 (considering shot noise only) or 3000 (noise from shape and large-scale-structure) massive clusters with a signal-to-noise ratio greater than 3.
2024-04-15
