Accès ouvert déclaré
2024
article
Euclid preparation
P. Hudelot, G. Seidel, Eric Jullo, F. Torradeflot, D. Benielli, R. Fahed, T. Auphan, J. Carretero, J. Davies, N. Fourmanoit, Stéphane Huot, S. Kermiche, K. Okumura, J. Zoubian, H. Bretonnière, B. Clément, C.A.J Duncan, Koshy George, M Kümmel, D. Laugier, G Mainetti, J. J. Mohr, A Montoro, C. Neissner, C. Rosset, M. Schirmer, A. Venhola, A. Verderi, A. Zacchei, N. Aghanim, B. Altieri, A. Amara, N. Auricchio, C. Baccigalupi, Marco Baldi, S Bardelli, Alberto Basset, Pietro Battaglia, F. Bernardeau, C. Bodendorf, D. Bonino, E Branchini, M. Brescia, S. Camera, Gian Paolo Candini, V. Capobianco, C. Carbone, Santiago Casas, M. Castellano, S. Cavuoti, R. Cledassou, G. Congedo, Christopher J. Conselice, L. Conversi, F. Courbin, M. Crocce, M. Cropper, H. Degaudenzi, A.M Di Giorgio, J. Dinis, F Dubath, X. Dupac, S Dusini, M. Farina, S. Farrens, S. Ferriol, M. Frailis, E. Franceschi, P. Franzetti, B. Garilli, W. Gillard, B. Gillis, C. Giocoli, B. R. Granett, A. Grazian, F. Grupp, S. V. H. Haugan, Henk Hoekstra, W. Holmes, I. Hook, K. Jahnkę, B. Joachimi, A. Kiessling, T. Kitching, R. Kohley, M. Kunz, Q Le Boulc'H, P. Liebing, S. Ligori, P. B. Lilje, V. Lindholm, I. Lloro, D. Maino, E. Maiorano, O Mansutti, S Marcin, O Marggraf, M. Martinelli, N. Martinet, R. Massey, S. Maurogordato, E. Medinaceli, S. Mei, M. Melchior, Y. Mellier, M. Meneghetti, E. Merlin, G. Meylan, M. Moresco, P. Morris, E. Munari, R. Nakajima, S.-M Niemi, T. Nutma, S. Paltani, F. Pasian, K. Pedersen, V. Pettorino, S. Pires, G. Polenta, L. A. Popa, L. Pozzetti, F. Raison, A. Renzi, Jason Rhodes, G. Riccio, E. Romelli, M. Roncarelli, E. Rossetti, B. Rusholme, R. P. Saglia, Z. Sakr, Ariel G. Sánchez, D Sapone, B. Sartoris, M. Sauvage, P. Schneider, M. Scodeggio, C. Sirignano, J. Skottfelt, L. Stanco, Jean‐Luc Starck, J. Steinwagner, H.I Teplitz, I. Tereno, R. Toledo-Moreo, I. Tutusaus, E. A. Valentijn, L. Valenziano, T. Vassallo, A Veropalumbo, Yun Wang, J. Weller, G. Zamorani, E. Zucca, A. Biviano, E. Bozzo, D. Di Ferdinando, R Farinelli, J. Graciá-Carpio, N. Mauri, V. Scottez, M. Tenti, Y. Akrami, V. Allevato, A. Blanchard, Alejandro S. Borlaff, S Bruton, C. Burigana, A. Cappi, C. S. Carvalho, T. Castro, J. Coupon, S. Davini, S. Desai, G. Desprez, A. Díaz‐Sánchez, H. Dole, J.A. Escartin Vigo, S. Escoffier, I. Ferrero, L. Gabarra, K. Ganga, J. García-Bellido, E. Gaztanaga, F. Giacomini, G. Gozaliasl, O. Ilbert, V. Kansal, J. F. Macías–Pérez, M. Magliocchetti, C.J.A.P. Martins, L. Maurin, M. Migliaccio, Pierluigi Monaco, G. Morgante, S. Nadathur, A. A. Nucita, M. Pöntinen, V. Popa, C. Porciani, D. Potter, M. Sereno, A. Shulevski, P. Šimon, A. Spurio Mancini, Joachim Stadel, M. Tewes, R. Teyssier, Sune Toft, M. Tucci, J Valiviita, I.A Zinchenko
10Citations signalées, ce qui n’est pas une note de qualité
139Institutions déclarées
20Pays d’affiliation déclarés
Rattachement africain : es, fr, de, bd, fi, us, ch, gb, it, pt, no, nl, dk, ca, ro, lb, cl, at, in, se.
Niveau de preuve : code pays fourni par la source.
Le résumé fourni par la source
Context. The European Space Agency’s Euclid mission is one of a raft of forthcoming large-scale cosmology surveys that will map the large-scale structure in the Universe with unprecedented precision. The mission will collect a vast amount of data that will be processed and analysed by Euclid ’s Science Ground Segment (SGS). The development and validation of the SGS pipeline requires state-of-the-art simulations with a high level of complexity and accuracy that include subtle instrumental features not accounted for previously as well as faster algorithms for the large-scale production of the expected Euclid data products. Aims. In this paper, we present the Euclid SGS simulation framework as it is applied in a large-scale end-to-end simulation exercise named Science Challenge 8. Our simulation pipeline enables the swift production of detailed image simulations for the construction and validation of the Euclid mission during its qualification phase and will serve as a reference throughout operations. Methods. Our end-to-end simulation framework started with the production of a large cosmological N-body simulation that we used to construct a realistic galaxy mock catalogue. We performed a selection of galaxies down to I E =26 and 28 mag, respectively, for a Euclid Wide Survey spanning 165 deg 2 and a 1 deg 2 Euclid Deep Survey. We built realistic stellar density catalogues containing Milky Way-like stars down to H < 26 from a combination of a stellar population synthesis model of the Galaxy and real bright stars. Using the latest instrumental models for both the Euclid instruments and spacecraft as well as Euclid -like observing sequences, we emulated with high fidelity Euclid satellite imaging throughout the mission’s lifetime. Results. We present the SC8 dataset, consisting of overlapping visible and near-infrared Euclid Wide Survey and Euclid Deep Survey imaging and low-resolution spectroscopy along with ground-based data in five optical bands. This extensive dataset enables end-to-end testing of the entire ground segment data reduction and science analysis pipeline as well as the Euclid mission infrastructure, paving the way for future scientific and technical developments and enhancements.
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
- 01/10/2024
- 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
Institute of Space SciencesInstitut d'Estudis Espacials de CatalunyaUniversitat Politècnica de CatalunyaCentre National de la Recherche ScientifiqueInstitut d'Astrophysique de ParisSorbonne UniversitéMax Planck Institute for AstronomyUniversité Paris CitéCommissariat à l'Énergie Atomique et aux Énergies AlternativesAstrophysique, Instrumentation et ModélisationCEA Paris-SaclayInstitut de Recherche sur les Lois Fondamentales de l'UniversAix-Marseille UniversitéPort d'Informació CientíficaCentro de Investigaciones Energéticas, Medioambientales y TecnológicasCentre de physique des particules de MarseilleInstitut National de Physique Nucléaire et de Physique des ParticulesInstitute for High Energy PhysicsUniversité Paris-SaclayCentre National d'Études SpatialesDamien FoundationUniversity of HelsinkiHelsinki Institute of PhysicsLyon 1 UniversitéInstitut de Physique des 2 Infinis de LyonUniversity of California, Santa CruzÉcole Polytechnique Fédérale de LausanneUniversity of ManchesterUniversity of OxfordLudwig-Maximilians-Universität MünchenCentre de Calcul de l’Institut National de Physique Nucléaire et de Physique des ParticulesMax Planck Institute for Extraterrestrial PhysicsUniversity of OuluTrieste Astronomical ObservatoryInstitute for Fundamental Physics of the UniverseInstitut d'Astrophysique SpatialeEuropean Space Astronomy CentreUniversity of PortsmouthBrera Astronomical ObservatoryOsservatorio di Astrofisica e Scienza dello SpazioUniversity College LondonScuola Internazionale Superiore di Studi AvanzatiUniversity of TriesteIstituto Nazionale di Fisica Nucleare, Sezione di TriesteIstituto Nazionale di Fisica Nucleare, Sezione di BolognaUniversity of BolognaInstitut de Physique ThéoriqueOsservatorio Astrofisico di TorinoIstituto Nazionale di Fisica Nucleare, Sezione di GenovaUniversity of GenoaAstronomical Observatory of CapodimonteFederico II University HospitalUniversidade do PortoInstitute of Astrophysics and Space SciencesIstituto Nazionale di Fisica Nucleare, Sezione di TorinoUniversity of TurinNational Institute for AstrophysicsRWTH Aachen UniversityAstronomical Observatory of RomeIstituto Nazionale di Fisica Nucleare, Sezione di NapoliInstituto de Astrofísica de CanariasRoyal ObservatoryUniversity of EdinburghEuropean Space Research InstituteUniversity of LisbonUniversity of GenevaInstitute for Space Astrophysics and PlanetologyIstituto Nazionale di Fisica Nucleare, Sezione di PadovaOsservatorio Astronomico di PadovaUniversity of MilanIstituto Nazionale di Fisica Nucleare, Sezione di MilanoUniversity of OsloLeiden UniversityJet Propulsion LaboratoryLancaster Universityvon Hoerner & Sulger (Germany)Technical University of DenmarkNetherlands Institute for Radio AstronomyFHNW University of Applied Sciences and Arts Northwestern SwitzerlandUniversity of BonnIstituto Nazionale di Fisica Nucleare, Sezione di Roma IDurham UniversityUniversité Côte d'AzurObservatoire de la Côte d’AzurCalifornia Institute of TechnologyEuropean Space Research and Technology CentreUniversity of GroningenAarhus UniversityUniversity of WaterlooPerimeter InstituteAgenzia Spaziale ItalianaInstitute of Space Science - INFLPR SubsidiaryUniversidad de La LagunaUniversity of PaduaInfrared Processing and Analysis CenterUniversité Toulouse III - Paul SabatierUniversité Fédérale de Toulouse Midi-PyrénéesSaint Joseph UniversityHeidelberg UniversityInstitut de Recherche en Astrophysique et PlanétologieHeidelberg Institute for Theoretical StudiesUniversity of ChileUniversität InnsbruckThe Open UniversityUniversidad Politécnica de CartagenaConsejo Superior de Investigaciones CientíficasUniversité Paris Sciences et LettresÉcole Normale Supérieure - PSLLaboratoire d’Etudes du Rayonnement et de la Matière en Astrophysique et AtmosphèresLaboratoire de Physique de l'Ecole Normale SupérieureImperial College LondonCase Western Reserve UniversityUniversidad Autónoma de MadridScuola Normale SuperioreUniversity of FerraraIstituto Nazionale di Fisica Nucleare, Sezione di FerraraAmes Research CenterKavli Institute for Particle Astrophysics and CosmologyStanford UniversityUniversity of MinnesotaIstituto di Radioastronomia di BolognaUniversity of Hawaii SystemUniversité Bourgogne Franche-ComtéUniversity of California, IrvineIndian Institute of Technology HyderabadSaint Mary's UniversityRuhr University BochumInstitut polytechnique de GrenobleUniversité Grenoble AlpesUniversity of TurkuStockholm UniversitySapienza University of RomeCentro de Astrofísica da Universidade do PortoUniversity of Rome Tor VergataUniversity of SalentoIstituto Nazionale di Fisica Nucleare, Sezione di LecceUniversity of ZurichPrinceton UniversityUniversity of Copenhagen
Une affiliation ne permet pas de déduire la nationalité d’un auteur.
Les sujets associés
Galaxies: Formation, Evolution, PhenomenaAstronomy and Astrophysical ResearchGamma-ray bursts and supernovae