Accès ouvert déclaré
2025
article
Euclid Quick Data Release (Q1)
H. (H.J) Mccracken, K Benson, C. Dolding, T. Flanet, C. Grenet, O. Hérent, P. Hudelot, C. Laigle, G Leroy, P. Liebing, R. Massey, S. Mottet, R. Nakajima, H.N. Nguyen-Kim, J.W Nightingale, J. Skottfelt, L. C. Smith, Franca Soldano, E. Vilenius, M Wander, Maximilian von Wietersheim-Kramsta, Mohammad Akhlaghi, H. Aussel, S. Awan, R. Azzollini, Alberto Basset, Gian Paolo Candini, P. Casenove, M. Cropper, Henk Hoekstra, H. Israel, Ali Kh. Khalil, K Kuijken, Y. Mellier, L. Miller, S.-M Niemi, M.J. Page, K. Paterson, M. Schirmer, N. A. Walton, A. Zacchei, J. Barrios, T. Erben, Robert B. Hayes, Jacob Kegerreis, David Lagattuta, A. Lançon, N. Aghanim, B. Altieri, A. Amara, S. Andreon, P. N. Appleton, N Auricchio, C. Baccigalupi, Marco Baldi, A. Balestra, S. Bardelli, P Battaglia, A. N. Belikov, R. Bender, Francis Bernardeau, A. Biviano, A Bonchi, E. Branchini, M. Brescia, J. Brinchmann, S. Camera, G Cañas-Herrera, V. Capobianco, C. Carbone, J. Carretero, Santiago Casas, F. J. Castander, M. Castellano, G. Castignani, S. Cavuoti, K. C. Chambers, A. Cimatti, C. Colodro-Conde, G. Congedo, C.J. Conselice, L. Conversi, Y. Copin, F. Courbin, H. M. Courtois, A. Da Silva, R. da Silva, H. Degaudenzi, G. De Lucia, A. M. Di Giorgio, J. Dinis, H. Dole, F Dubath, X. Dupac, S. Dusini, A. Ealet, S. Escoffier, M. Fabricius, M. Farina, R Farinelli, S Ferriol, F. Finelli⋆, P. Fosalba, S. Fotopoulou, N. Fourmanoit, M. Frailis, E. Franceschi, S. Galeotta, Koshy George, W. Gillard, B Gillis, C. Giocoli, P. Gómez-Álvarez, J. Gracia-Carpio, B. R. Granett, A. Grazian, F. Grupp, L. Guzzo, M. Hailey, S. V. H. Haugan, J. Hoar, W. A. Holmes, F. Hormuth, A. Hornstrup, K. Jahnkę, M. Jhabvala, B Joachimi, E. Keihänen, S. Kermiche, A. Kiessling, M. Kilbinger, B. Kubik, M. Kümmel, M. Kunz, H Kurki-Suonio, Q. Le Boulc'h, A.M.C Le Brun, D. Le Mignant, S. Ligori, P. B. Lilje, V. Lindholm, I. Lloro, G Mainetti, E. Maiorano, E Maiorano, O. Mansutti, S. Marcin, O Marggraf, M. Martinelli, N. Martinet, F. Marulli, Daniel Masters, S. Maurogordato, E. Medinaceli, S. Mei, M. Melchior, M. Meneghetti, E Merlin, G. Meylan, A. Mora, M. Moresco, L. Moscardini, C. Neissner, R. C. Nichol, C. Padilla, S. Paltani, F. Pasian, K. Pedersen, Will J. Percival, V. Pettorino, S Pires, G. Polenta, M. Poncet, Popa LG, L. Pozzetti, Giuseppe D. Racca, F. Raison, R. Rébolo, A. Renzi, Jason Rhodes, G. Riccio, E. Romelli, M. Roncarelli, E. Rossetti, B. Rusholme, R. P. Saglia, Z. Sakr, A.G. Sánchez, D Sapone, B. Sartoris, J.A Schewtschenko, P. C. Schneider, T. Schrabback, A. Secroun, G Seidel, M. D. Seiffert, S Serrano, Patrice Simon, C. Sirignano, G. Sirri, A. Spurio Mancini, L. Stanco, J. Steinwagner, P. Tallada-Crespí, D. Tavagnacco, A.N. Taylor, Harry I. Teplitz, I Tereno, N Tessore, Sune Toft, R. Toledo-Moreo, F. Torradeflot, I. Tutusaus, E. A. Valentijn, L. Valenziano, J. Väliviita, T. Vassallo, G. Verdoes Kleijn, A. Veropalumbo, Yun Wang, J. Weller, G. Zamorani, F. M. Zerbi, I. A. Zinchenko, E. Zucca, V. Allevato, M. Ballardini, M. Bolzonella, E. Bozzo, 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, I Risso, V Scottez, M. Sereno, M. Tenti, Matteo Viel, M. Wiesmann, Y. Akrami, I.T Andika, S Anselmi, M. Archidiacono, F. Atrio‐Barandela, Christophe Benoıst, P. Bergamini, Daniele Bertacca, M. Béthermin, L Bisigello, Alain Blanchard, L Blot, S Borgani, Alejandro S. Borlaff, M.L Brown, S Bruton, A Calabrò, B. Camacho Quevedo, F Caro, C.S. Carvalho, T. Castro, F Cogato, Simon Conseil, A.R. Cooray, O. Cucciati, S. Davini, F. De Paolis, G. Desprez, A. Díaz‐Sánchez, J.J Diaz, S. Di Domizio, J. M. Diego, P.‐A. Duc, A Enia, Yuhong Fang, A. M. N. Ferguson, A.G Ferrari, A. Finoguenov, A. Fontana, A Franco, K. Ganga, J. García-Bellido, T Gasparetto, V Gautard, E. Gaztañaga, F. Giacomini, F. Gianotti, A.H. Gonzalez, G. Gozaliasl, A. Gregorio, M Guidi, C. M. Gutiérrez, Alex Hall, W.G Hartley, C. Hernández–Monteagudo, H. Hildebrandt, J. Hjorth, J. J. E. Kajava, Y. W. Kang, V. Kansal, D. Karagiannis, K Kiiveri, C. C. Kirkpatrick, Sandor Kruk, J Le Graet, L. Legrand, Maria Lembo, F Lepori, G.F Lesci, J. Lesgourgues, L. Leuzzi, T.I Liaudat, S.J Liu, A. Loureiro, J. F. Macías–Pérez, G. Maggio, M. Magliocchetti, F. Mannucci, R. Maoli, C.J.A.P. Martins, L. Maurin, Conor McPartland, M Miluzio, P. Monaco, A Montoro, Claudio Moretti, G Morgante, Clare Murray, S. Nadathur, Krishna Naidoo, A. Navarro-Alsina, S Nesseris, F Passalacqua, L. Patrizii, A. Pisani, D. Potter, S Quai, M. Radovich, P. Reimberg, P.-F Rocci, G. Rodighiero, R. P. Rollins, S Sacquegna, M Sahlén, D. B. Sanders, E Sarpa, Claudia Scarlata, Aurel Schneider, M. Schultheis, D Sciotti, E. Sellentin, Francesco Shankar, Alessandra Silvestri, K Tanidis, Chunhui Tao, G. Testera, M. Tewes, Romain Teyssier, S. Tosi, A. Troja, M. Tucci, C Valieri, A. Venhola, D. Vergani, G Verza, P Vielzeuf, John R. Weaver, D. Scott
22Citations signalées, ce qui n’est pas une note de qualité
169Institutions déclarées
26Pays d’affiliation déclarés
Rattachement africain : fr, gb, de, my, ru, es, nl, us, it, sk, pt, ch, ca, no, dk, fi, lb, cz, ro, cl, at, jp, au, Afrique du Sud, se, uz.
Niveau de preuve : code pays fourni par la source.
Le résumé fourni par la source
This paper describes the VIS processing function (VIS PF) of the Euclid ground segment pipeline, which processes and calibrates raw data from the VIS camera. We present the algorithms used in each processing element along with a description of the on-orbit performance of VIS PF based on performance verification and Q1 datasets. We demonstrate that the principal performance metrics (image quality, astrometric accuracy, photometric calibration) are within pre-launch specifications. The image-to-image photometric scatter is less than 0.8% and absolute astrometric accuracy compared to Gaia is 5 mas. Image quality is stable over all Q1 images, with a full width at half maximum (FWHM) of 0 . ″ 16. The stacked images (combining four nominal and two short exposures) reach I E = 25.6 (10 σ , measured as the variance of 1 . ″ 3 diameter apertures). We also describe quality control metrics provided with each image, and an appendix provides a detailed description of the provided data products. The excellent quality of these images demonstrates the immense potential of Euclid VIS data for weak lensing. VIS data covering most of the extragalactic sky will provide a lasting high-resolution atlas of the Universe.
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 ; titre concordant.
- Titre Crossref
- Euclid Quick Data Release (Q1)
- Date Crossref
- 30/06/2026
- 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
Centre National de la Recherche ScientifiqueInstitut d'Astrophysique de ParisSorbonne UniversitéUniversity College LondonDurham UniversityUniversity of BonnNewcastle UniversityOpen University MalaysiaUniversity of CambridgeInstitute of AstronomyCentro de Estudios de Física del Cosmos de AragónUniversité Paris CitéCommissariat à l'Énergie Atomique et aux Énergies AlternativesUniversité Paris-SaclayAstrophysique, Instrumentation et ModélisationCEA Paris-SaclayCentre National d'Études SpatialesLeiden UniversityIsland Peer Review OrganizationUniversity of OxfordEuropean Space AgencyEuropean Space Research and Technology CentreMax Planck Institute for AstronomyTrieste Astronomical ObservatoryInstitute for Fundamental Physics of the UniverseAmes Research CenterObservatoire astronomique de StrasbourgInstitut d'Astrophysique SpatialeEngineering Science Analysis (United States)University of SurreyBrera Astronomical ObservatoryCalifornia Institute of TechnologyInfrared Processing and Analysis CenterOsservatorio di Astrofisica e Scienza dello SpazioScuola Internazionale Superiore di Studi AvanzatiIstituto Nazionale di Fisica Nucleare, Sezione di TriesteOsservatorio astronomico di BolognaIstituto Nazionale di Fisica Nucleare, Sezione di BolognaUniversity of BolognaOsservatorio Astronomico di PadovaUniversity of GroningenATG Europe (Netherlands)Astronomical Institute of the Slovak Academy of SciencesMax Planck Institute for Extraterrestrial PhysicsLudwig-Maximilians-Universität MünchenInstitut de Physique ThéoriqueUnited Kingdom Space AgencyIstituto 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 TorinoOsservatorio Astrofisico di TorinoUniversity of TurinNational Institute for AstrophysicsPort d'Informació CientíficaCentro de Investigaciones Energéticas, Medioambientales y TecnológicasRWTH Aachen UniversityInstitute of Space SciencesInstitut d'Estudis Espacials de CatalunyaAstronomical Observatory of RomeIstituto Nazionale di Fisica Nucleare, Sezione di NapoliNaples Anesthesia & Physician AssociatesUniversity of Hawaii SystemInstituto de Astrofísica de CanariasRoyal ObservatoryUniversity of EdinburghSKA ObservatoryEuropean Space Research InstituteLyon 1 UniversitéInstitut 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 PlanetologyIstituto Nazionale di Fisica Nucleare, Sezione di PadovaAix-Marseille UniversitéCentre de physique des particules de MarseilleUniversity of BristolBristol Robotics LaboratoryFractal Systems (Canada)University of MilanIstituto Nazionale di Fisica Nucleare, Sezione di MilanoUniversity of OsloJet Propulsion LaboratoryFelix ScholarshipDAWN Center for Independent LivingTechnical University of DenmarkGoddard Space Flight CenterUniversity of HelsinkiHelsinki Institute of PhysicsLaboratoire de Physique ThéoriqueCentre de Calcul de l’Institut National de Physique Nucléaire et de Physique des ParticulesUniversité Paris Sciences et LettresFHNW University of Applied Sciences and Arts Northwestern SwitzerlandIstituto Nazionale di Fisica Nucleare, Sezione di Roma IUniversité Côte d'AzurObservatoire de la Côte d’AzurInternational University of BeirutFZU ‒ Institute of Physics of the Academy of Sciences of the Czech RepublicÉcole Polytechnique Fédérale de LausanneInstitute for High Energy PhysicsUniversity of CopenhagenUniversity of WaterlooPerimeter InstituteInstitute of Space Science - INFLPR SubsidiaryConsejo Superior de Investigaciones CientíficasUniversidad de La LagunaUnidades Centrales Científico-TécnicasUniversity of PaduaUniversité Toulouse III - Paul SabatierUniversité Fédérale de Toulouse Midi-PyrénéesUniversity of Saint JosephHeidelberg UniversitySt. Joseph Medical CenterInstitut de Recherche en Astrophysique et PlanétologieHeidelberg Institute for Theoretical StudiesUniversity of ChileUniversität InnsbruckGenlantis (United States)Royal Holloway University of LondonUniversidad Politécnica de CartagenaUniversity of FerraraIstituto Nazionale di Fisica Nucleare, Sezione di FerraraIstituto di Radioastronomia di BolognaOsservatorio Astronomico della Regione Autonoma Valle d'AostaCardiff UniversityUniversité Catholique de LilleComputing CenterCase Western Reserve UniversityMax Planck Institute for AstrophysicsTechnical University of MunichSorbonne Paris CitéUniversidad de SalamancaKavli Institute for the Physics and Mathematics of the UniverseBay Area Environmental Research InstituteUniversity of California, IrvineUniversity of SalentoIstituto Nazionale di Fisica Nucleare, Sezione di LecceInstituto de Física de CantabriaInstitut de Recherche sur les Lois Fondamentales de l'UniversUniversity of PortsmouthAstronomy and SpaceAalto UniversityUniversity of TurkuARC Centre of Excellence for Dark Matter Particle PhysicsSwinburne University of TechnologyUniversity of the Western CapeUniversity of ZurichStockholm UniversityImperial College LondonInstitut polytechnique de GrenobleInstitut National de Physique Nucléaire et de Physique des ParticulesUniversité Grenoble AlpesArcetri Astrophysical ObservatorySapienza University of RomeCentro de Astrofísica da Universidade do PortoPrinceton UniversityCentre for Theoretical Physics and AstrophysicsUniversity of MinnesotaMathematical Institute of the Slovak Academy of SciencesUniversity of SouthamptonFlatiron Health (United States)Flatiron InstituteUniversity of British Columbia
Une affiliation ne permet pas de déduire la nationalité d’un auteur.
Les sujets associés
Galaxies: Formation, Evolution, PhenomenaAstronomy and Astrophysical ResearchCCD and CMOS Imaging Sensors