Accès ouvert déclaré
2025
article
Euclid preparation
Pierluigi Monaco, Gabriele Parimbelli, M.Y Elkhashab, J. Salvalaggio, T. Castro, M.D Lepinzan, E Sarpa, E Sefusatti, L. Stanco, L. Tornatore, Graeme E. Addison, S Bruton, C. Carbone, F. J. Castander, J. Carretero, S. de la Torre, P Fosalba, Guilhem Lavaux, S Lee, K. Markovič, Kevin S. McCarthy, F Passalacqua, Will J. Percival, I Risso, Claudia Scarlata, P. Tallada-Crespí, Matteo Viel, Yun Wang, B. Altieri, S. Andreon, N. Auricchio, C. Baccigalupi, M. Baldi, S. Bardelli, P Battaglia, Francis Bernardeau, A. Biviano, E. Branchini, M. Brescia, J. Brinchmann, S. Camera, G Cañas-Herrera, V. Capobianco, V. F. Cardone, S Casas, M. Castellano, G. Castignani, S. Cavuoti, A. Cimatti, C Colodro-Conde, G. Congedo, Christopher J. Conselice, L Conversi, Y. Copin, F. Courbin, H. M. Courtois, A. Da Silva, H. Degaudenzi, G. De Lucia, A. M. Di Giorgio, F. Dubath, Franck Ducret, C. A. J. Duncan, X. Dupac, S Dusini, A. Ealet, S. Escoffier, M. Farina, R. Farinelli, S Farrens, S Ferriol, F. Finelli⋆, N. Fourmanoit, M. Frailis, E. Franceschi, M. Fumana, S. Galeotta, Koshy George, B. Gillis, C. Giocoli, J Gracia-Carpio, A. Grazian, F Grupp, L. Guzzo, S. V. H. Haugan, W. A. Holmes, F Hormuth, A. Hornstrup, K. Jahnkę, M. Jhabvala, B Joachimi, E. Keihänen, S. Kermiche, B. Kubik, M Kümmel, M. Kunz, H. Kurki‐Suonio, A.M.C Le Brun, S. Ligori, P. B. Lilje, V. Lindholm, I. Lloro, D Maino, E. Maiorano, O. Mansutti, O. Marggraf, M. Martinelli, N. Martinet, F. Marulli, R. Massey, E. Medinaceli, S. Mei, M. Melchior, Y. Mellier, M. Meneghetti, E Merlin, G Meylan, A. Mora, M. Moresco, L. Moscardini, E. Munari, R. Nakajima, C. Neissner, S.-M. Niemi, C. Padilla Aranda, S Paltani, F. Pasian, Kim Steenstrup Pedersen, V. Pettorino, S. Pires, G. Polenta, M Poncet, L. A. Popa, L. Pozzetti, F. Raison, A. Renzi, J. Rhodes, G. Riccio, F. Rizzo, E. Romelli, M. Roncarelli, R. P. Saglia, Z. Sakr, Ariel G. Sánchez, D. Sapone, B. Sartoris, P Schneider, T. Schrabback, M. Scodeggio, A. Secroun, G. Seidel, M. D. Seiffert, S. Serrano, P Simon, C. Sirignano, G. Sirri, J Steinwagner, D. Tavagnacco, A. J. Taylor, I. Tereno, N Tessore, Sune Toft, R. Toledo-Moreo, F Torradeflot, I. Tutusaus, L. Valenziano, J. Väliviita, T. Vassallo, G. Verdoes Kleijn, A. Veropalumbo, J. Weller, G. Zamorani, E. Zucca, V. Allevato, M. Ballardini, C. Burigana, R. Cabanac, M. Calabrese, A Cappi, D. Di Ferdinando, J.A. Escartin Vigo, Giulio Fabbian, L. Gabarra, J Martín-Fleitas, S Matthew, N. Mauri, R. B. Metcalf, A Pezzotta, M. Pöntinen, C. Porciani, V Scottez, M. Sereno, M. Tenti, M. Wiesmann, Y. Akrami, S Alvi, I.T Andika, S Anselmi, Maria Archidiacono, F. Atrio‐Barandela, S. Àvila, A. Balaguera-Antolínez, P. Bergamini, Daniele Bertacca, M. Béthermin, Alain Blanchard, L Blot, S. Borgani, Michael D. Brown, Anthony Calabro, B. Camacho Quevedo, F Caro, Carvalho C, F Cogato, Simon Conseil, S. Contarini, Asantha Cooray, O. Cucciati, S. Davini, G. Desprez, A. Díaz‐Sánchez, J.J Diaz, S. Di Domizio, J. M. Diego, A Enia, Y D Fang, A.G Ferrari, A Finoguenov, Fabio Fontanot, A Franco, K. Ganga, J. García-Bellido, T Gasparetto, V Gautard, E. Gaztañaga, F. Giacomini, F. Gianotti, G. Gozaliasl, M Guidi, C. M. Gutiérrez, A Hall, Shoubaneh Hemmati, C. Hernández-Monteagudo, H. Hildebrandt, J. Hjorth, Shahab Joudaki, J. J. E. Kajava, Y Kang, V. Kansal, D. Karagiannis, K. Kiiveri, C. C. Kirkpatrick, Sandor Kruk, V. Le Brun, J Le Graet, L. Legrand, Maria Lembo, Francesca Lepori, Gavin Leroy, G. F. Lesci, Julien Lesgourgues, L. Leuzzi, T.I Liaudat, J. F. Macías–Pérez, G. Maggio, M. Magliocchetti, C. Mancini, F. Mannucci, R. Maoli, C. J. A. P. Martins, L. Maurin, M Miluzio, A Montoro, Claudio Moretti, G. Morgante, S. Nadathur, Krishna Naidoo, A Navarro-Alsina, Savvas Nesseris, K. Paterson, Alice Pisani, D. Potter, S Quai, M. Radovich, G. Rodighiero, S Sacquegna, M Sahlén, D. B. Sanders, D Sciotti, Elena Sellentin, Leigh C. Smith, J. G. Sorce, G. Testera, C. Tao, G. Testera, Romain Teyssier, S. Tosi, A. Troja, M. Tucci, C Valieri, A. Venhola, Filippo Vernizzi, G Verza, P Vielzeuf, N. A. Walton
5Citations signalées, ce qui n’est pas une note de qualité
164Institutions déclarées
23Pays d’affiliation déclarés
Rattachement africain : it, es, us, fr, jp, ca, pt, nl, de, gb, ch, rs, no, dk, fi, ro, cl, at, sk, au, Afrique du Sud, uz, ru.
Niveau de preuve : code pays fourni par la source.
Le résumé fourni par la source
We present two extensive sets of 3500+1000 simulations of dark matter haloes on the past light cone and two corresponding sets of simulated (mock) galaxy catalogues that represent the spectroscopic sample of Euclid . The simulations were produced with the latest version of the code Pinocchio and provide the largest public set of simulated skies. The mock galaxy catalogues were obtained by populating haloes with galaxies using an halo occupation distribution (HOD) model extracted from the Flagship galaxy catalogue provided by Euclid Collaboration. The Geppetto set of 3500 simulated skies was obtained by tiling a 1.2 h −1 Gpc box to cover a light cone whose sky footprint is a circle with a radius of 30° for an area of 2763 deg 2 and a minimum halo mass of 1.5 × 10 11 h −1 M ⊙ . The relatively small size of the box means that this set is unsuitable for measuring very large scales. The EuclidLargeBox set consists of 1000 simulations of 3.38 h −1 Gpc and has the same mass resolution and a footprint that covers half of the sky. It excludes the Milky Way zone of avoidance. From this, we produced a set of 1000 EuclidLargeMocks on the 30° radius footprint, whose comoving volume is fully contained in the simulation box. We validated the two sets of catalogues by analysing number densities, power spectra, and two-point correlation functions to show that the Flagship spectroscopic catalogue is consistent with being one of the realisations of the simulated sets. We noted small deviations, however, that are limited to the quadrupole at k > 0.2 h Mpc −1 . We infer the cosmological parameters from these catalogues and demonstrate that using one realisation of EuclidLargeMocks in place of the Flagship mock produces the same posteriors to within the expected shift given by the sample variance. These simulated skies will be used for the galaxy clustering analysis of the Euclid Data Release 1 (DR1), and an even larger set of simulations is planned for the next releases.
Ce résumé expose les affirmations des auteurs. BNTIC ne l’interprète pas comme une validation indépendante des résultats.
Le contrôle bibliographique ouvert
DOI retrouvé dans Crossref DOI retrouvé, mais le titre doit être comparé manuellement.
- Titre Crossref
- <i>Euclid</i>
preparation
- Date Crossref
- 01/12/2025
- Éditeur
- EDP Sciences
- Type
- journal-article
Ce recoupement confirme des métadonnées liées au DOI. Il ne confirme ni la méthode ni les conclusions de l’étude, et il ne compte pas comme une seconde source scientifique indépendante.
Les institutions déclarées
Trieste Astronomical ObservatoryInstitute for High Performance Computing and NetworkingIstituto Nazionale di Fisica Nucleare, Sezione di TriesteScuola Internazionale Superiore di Studi AvanzatiInstitute of Space SciencesIstituto Nazionale di Fisica Nucleare, Sezione di GenovaInstitute for Fundamental Physics of the UniverseIstituto Nazionale di Fisica Nucleare, Sezione di PadovaJohns Hopkins UniversityCalifornia Institute of TechnologyNational Institute for AstrophysicsInstitut d'Estudis Espacials de CatalunyaPort d'Informació CientíficaCentro de Investigaciones Energéticas, Medioambientales y TecnológicasAix-Marseille UniversitéLaboratoire d’Astrophysique de MarseilleChâteau GombertCentre National de la Recherche ScientifiqueInstitut d'Astrophysique de ParisSorbonne UniversitéJet Propulsion LaboratoryKavli Institute for the Physics and Mathematics of the UniverseUniversity of PaduaUniversity of WaterlooPerimeter InstituteBrera Astronomical ObservatoryUniversity of MinnesotaInfrared Processing and Analysis CenterEuropean Space Astronomy CentreOsservatorio di Astrofisica e Scienza dello SpazioOsservatorio astronomico di BolognaIstituto Nazionale di Fisica Nucleare, Sezione di BolognaUniversity of BolognaCommissariat à l'Énergie Atomique et aux Énergies AlternativesCEA Paris-SaclayInstitut de Physique ThéoriqueUniversity of GenoaAstronomical Observatory of CapodimonteFederico II University HospitalUniversidade do PortoInstitute of Astrophysics and Space SciencesIstituto Nazionale di Fisica Nucleare, Sezione di TorinoOsservatorio Astrofisico di TorinoUniversity of TurinLeiden UniversityEuropean Space AgencyEuropean Space Research and Technology CentreAstronomical Observatory of RomeIstituto Nazionale di Fisica Nucleare, Sezione di Roma IRWTH Aachen UniversityIstituto Nazionale di Fisica Nucleare, Sezione di NapoliNaples Anesthesia & Physician AssociatesInstituto de Astrofísica de CanariasRoyal ObservatoryUniversity of EdinburghSKA ObservatoryEuropean Space Research InstituteLyon 1 UniversitéInstitute of Nuclear Physics of LyonInstitut de Physique des 2 Infinis de LyonInstitució Catalana de Recerca i Estudis AvançatsInstitut Català de Ciències del ClimaLyon CollegeUniversity of LisbonUniversity of GenevaInstitute for Space Astrophysics and PlanetologyCentre de physique des particules de MarseilleAstrophysique, Instrumentation et ModélisationUniversité Paris CitéUniversité Paris-SaclayAstronomical ObservatoryMax Planck Institute for Extraterrestrial PhysicsOsservatorio Astronomico di PadovaLudwig-Maximilians-Universität MünchenUniversity of MilanIstituto Nazionale di Fisica Nucleare, Sezione di MilanoUniversity of OsloFelix ScholarshipDAWN Center for Independent LivingTechnical University of DenmarkMax Planck Institute for AstronomyGoddard Space Flight CenterUniversity College LondonLaboratoire de Physique ThéoriqueObservatoire de ParisHelsinki Institute of PhysicsLaboratoire Univers et ThéoriesUniversité Paris Sciences et LettresUniversity of BonnFHNW University of Applied Sciences and Arts Northwestern SwitzerlandÉcole Polytechnique Fédérale de LausanneInstitute for High Energy PhysicsUniversity of CopenhagenCentre National d'Études SpatialesUnited Kingdom Space AgencyInstitute of Space Science - INFLPR SubsidiaryInstitut de Recherche en Astrophysique et PlanétologieUniversité Toulouse III - Paul SabatierUniversité Fédérale de Toulouse Midi-PyrénéesUniversity of Saint JosephHeidelberg UniversitySt. Joseph Medical CenterHeidelberg Institute for Theoretical StudiesUniversity of ChileUniversität InnsbruckPark UniversityUniversidad Politécnica de CartagenaUniversity of GroningenAstronomical Institute of the Slovak Academy of SciencesUniversity of FerraraIstituto Nazionale di Fisica Nucleare, Sezione di FerraraIstituto di Radioastronomia di BolognaLagrange LaboratoryOsservatorio Astronomico della Regione Autonoma Valle d'AostaObservatoire de la Côte d’AzurInstitut d'Astrophysique SpatialeCardiff UniversityUniversity of OxfordUniversité de LilleUniversité Catholique de LilleConsejo Superior de Investigaciones CientíficasCase Western Reserve UniversityJanssen (France)Max Planck Institute for AstrophysicsTechnical University of MunichSorbonne Paris CitéUniversidad de SalamancaObservatoire astronomique de StrasbourgUniversity of California, IrvineInstituto de Física de CantabriaUniversity of SalentoIstituto Nazionale di Fisica Nucleare, Sezione di LecceCEA GrenobleCEA CadaracheInstitut de Recherche sur les Lois Fondamentales de l'UniversUniversity of PortsmouthAalto UniversityIAC (United States)Universidad de La LagunaARC Centre of Excellence for Dark Matter Particle PhysicsSwinburne University of TechnologyUniversity of the Western CapeUniversity of ZurichDurham UniversityLaboratoire de Physique Subatomique et de CosmologieInstitut polytechnique de GrenobleInstitut National de Physique Nucléaire et de Physique des ParticulesUniversité Grenoble AlpesArcetri Astrophysical ObservatorySapienza University of RomeCentro de Astrofísica da Universidade do PortoCollurania Teramo ObservatoryCentre for Theoretical Physics and AstrophysicsUniversity of Hawaii SystemCentre de Recherche en InformatiqueMathematical Institute of the Slovak Academy of SciencesCentre de Recherche en Informatique, Signal et Automatique de LilleUniversity of CambridgeInstitute of AstronomyÉcole Centrale de LillePrinceton UniversityAstronomy and SpaceFlatiron Health (United States)Flatiron Institute
Une affiliation ne permet pas de déduire la nationalité d’un auteur.
Les sujets associés
Scientific Computing and Data ManagementSimulation Techniques and ApplicationsComputer Graphics and Visualization Techniques