Accès ouvert déclaré
2025
article
Euclid Quick Data Release (Q1)
G. Polenta, M. Frailis, Anahita Alavi, P. N. Appleton, Petra Awad, A Bonchi, R. J. Bouwens, L. Bramante, D. Busonero, G. Calderone, F Cogato, Simon Conseil, M. Correnti, R da Silva, I. Das, F Faustini, Y. Fu, T Gasparetto, W. Gillard, A Grazian, Shoubaneh Hemmati, J. Jacobson, K. Jahnkę, B. Kubik, X. Liu, C. Macabiau, E. Medinaceli, P. Morris, K. Paterson, M. Radovich, M. Schirmer, A. Shulevski, H.I Teplitz, B. Venemans, N. Aghanim, B. Altieri, A. Amara, S. Andreon, N. Auricchio, H. Aussel, C. Baccigalupi, M. Baldi, A. Balestra, S. Bardelli, Alberto Basset, P Battaglia, A. N. Belikov, R. Bender, A. Biviano, E Branchini, M. Brescia, J. Brinchmann, A. Caillat, S Camera, G Cañas-Herrera, V. Capobianco, C. Carbone, J. Carretero, S. 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, L. Corcione, A. Costille, F. Courbin, H. M. Courtois, A. Da Silva, H. Degaudenzi, G. De Lucia, A. M. Di Giorgio, H. Dole, F. Dubath, C. A. J. Duncan, X. Dupac, S Dusini, A. Ealet, S. Escoffier, Maximilian Fabricius, M. Farina, R. Farinelli, S. Ferriol, F. Finelli⋆, S. Fotopoulou, N. Fourmanoit, E. Franceschi, M. Fumana, S. Galeotta, K. George, B. Gillis, C. Giocoli, P. Gómez-Álvarez, J. Gracia-Carpio, B. R. Granett, F Grupp, S. V. H. Haugan, J. Hoar, H Hoekstra, W. Holmes, I. Hook, F. Hormuth, A. Hornstrup, P. Hudelot, M. Jhabvala, E. Keihänen, S. Kermiche, A. Kiessling, K Kuijken, M Kümmel, M. Kunz, H. Kurki‐Suonio, Q. Le Boulc'h, A.M.C Le Brun, D. Le Mignant, P. Liebing, S. Ligori, P. B. Lilje, V. Lindholm, I. Lloro, G Mainetti, D. Maino, E. Maiorano, O. Mansutti, S. Marcin, O. Marggraf, M. Martinelli, N. Martinet, F. Marulli, R. Massey, S. Maurogordato, H. J. McCracken, S. Mei, M. Melchior, Y. Mellier, M. Meneghetti, E. Merlin, G. Meylan, A Mora, M. Moresco, L. Moscardini, R. Nakajima, C. Neissner, R. C. Nichol, S.-M Niemi, J.W Nightingale, C Padilla, S. Paltani, F. Pasian, K. Pedersen, Will J. Percival, V. Pettorino, S. Pires, M. Poncet, L. A. Popa, L. Pozzetti, Giuseppe D. Racca, F. Raison, R. Rébolo, A. Renzi, J. 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. Schneider, M. Scodeggio, A. Secroun, E. Sefusatti, G. Seidel, M. D. Seiffert, S. Serrano, Pardis Simon, C. Sirignano, G. Sirri, A. Spurio Mancini, L Stanco, J. Steinwagner, P. Tallada-Crespí, D. Tavagnacco, A.N. Taylor, 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, A. Zacchei, 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, P Casenove, D. Di Ferdinando, J.A. Escartin Vigo, G. Fabbian, L. Gabarra, J Martín-Fleitas, S Matthew, N. Mauri, Achille Nucita, A Pezzotta, M. Pöntinen, C. Porciani, I Risso, V. Scottez, M. Sereno, M. Tenti, M. Viel, M. Wiesmann, Y. Akrami, I.T Andika, S Anselmi, M. Archidiacono, F. Atrio‐Barandela, Christophe Benoıst, P. Bergamini, Daniele Bertacca, M. Béthermin, G. Rodighiero, Alain Blanchard, L Blot, S Borgani, Alejandro S. Borlaff, M.L Brown, S Bruton, Antonello Calabrò, B. Camacho Quevedo, F Caro, C.S. Carvalho, T. Castro, Yann Philippe Charles, R. Chary, 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, P.G Ferreira, A. Finoguenov, A. Fontana, A. Franco, K. Ganga, J. García-Bellido, V Gautard, E. Gaztañaga, F. Giacomini, F. Gianotti, Anthony H. Gonzalez, G. Gozaliasl, A. Gregorio, A. Gruppuso, M Guidi, C. M. Gutiérrez, A 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, V. Le Brun, J Le Graet, L. Legrand, Maria Lembo, F Lepori, G Leroy, G.F Lesci, Julien 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, Chiara Moretti, G Morgante, S. Nadathur, Krishna Naidoo, P. Natoli, A. Navarro-Alsina, S Nesseris, L. Nicastro, F Passalacqua, L. Patrizii, A. Pisani, D. Potter, S Quai, P.-F Rocci, G. Rodighiero, S Sacquegna, M Sahlén, D. B. Sanders, E Sarpa, C. Scarlata, Aurel Schneider, D Sciotti, E. Sellentin, Francesco Shankar, L. C. Smith, G. Testera, C. Tao, G. Testera, Romain Teyssier, S. Tosi, A. Troja, M. Tucci, C Valieri, A. Venhola, D. Vergani, G Verza, P Vielzeuf, N. A. Walton, John R. Weaver, M. Bella, D. Scott
17Citations signalées, ce qui n’est pas une note de qualité
165Institutions déclarées
24Pays d’affiliation déclarés
Rattachement africain : fr, gb, it, us, nl, sk, de, mk, pt, es, ch, ca, no, dk, fi, lb, ro, cl, au, ru, jp, Afrique du Sud, se, uz.
Niveau de preuve : code pays fourni par la source.
Le résumé fourni par la source
This paper describes the near-infrared processing function (NIR PF) that processes NIR images from the Near-Infrared Spectrometer and Photometer (NISP) instrument on board the Euclid satellite. NIR PF consists of three main components: (i) a common pre-processing stage for both photometric (NIR) and spectroscopic (SIR) data to remove instrumental effects; (ii) astrometric and photometric calibration of NIR data, along with catalogue extraction; and (iii) resampling and stacking. The necessary calibration products are generated using dedicated pipelines that process observations from both the early performance verification (PV) phase in 2023 and the nominal survey operations. After outlining the pipelineś structure and algorithms, we describe its application to Euclid Q1 images. For Q1, we achieved an astrometric accuracy of 5–8 mas, a relative photometric accuracy of 5 mmag, along with an absolute flux calibration limited by the 1% uncertainty of the Hubble Space Telescope (HST) CALSPEC database. We characterised the point spread function (PSF), which we found to be very stable across the focal plane. Finally, we discuss current limitations of NIR PF that will be improved upon for future data 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 ; 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
European Space AgencyUnited Kingdom Space AgencyTrieste Astronomical ObservatoryCalifornia Institute of TechnologyInfrared Processing and Analysis CenterLeiden UniversityLogistics Management Institute (United States)Osservatorio Astrofisico di TorinoOsservatorio di Astrofisica e Scienza dello SpazioUniversity of BolognaLyon 1 UniversitéCentre National de la Recherche ScientifiqueInstitut de Physique des 2 Infinis de LyonAstronomical Observatory of RomeNational Institute for AstrophysicsUniversity of GroningenAstronomical Institute of the Slovak Academy of SciencesAix-Marseille UniversitéCentre de physique des particules de MarseilleOsservatorio Astronomico di PadovaMax Planck Institute for AstronomySs. Cyril and Methodius University in SkopjeUniversity of AmsterdamNetherlands Institute for Radio AstronomyUniversité Paris-SaclayInstitut d'Astrophysique SpatialeEngineering Science Analysis (United States)University of SurreyBrera Astronomical ObservatoryUniversité Paris CitéCommissariat à l'Énergie Atomique et aux Énergies AlternativesAstrophysique, Instrumentation et ModélisationCEA Paris-SaclayScuola Internazionale Superiore di Studi AvanzatiIstituto Nazionale di Fisica Nucleare, Sezione di TriesteInstitute for Fundamental Physics of the UniverseOsservatorio astronomico di BolognaIstituto Nazionale di Fisica Nucleare, Sezione di BolognaCentre National d'Études SpatialesATG Europe (Netherlands)Max Planck Institute for Extraterrestrial PhysicsLudwig-Maximilians-Universität MünchenIstituto 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 TurinEuropean Space Research and Technology CentrePort d'Informació CientíficaCentro de Investigaciones Energéticas, Medioambientales y TecnológicasRWTH Aachen UniversityInstitut d'Estudis Espacials de CatalunyaInstitute of Space SciencesIstituto Nazionale di Fisica Nucleare, Sezione di NapoliNaples Anesthesia & Physician AssociatesUniversity of Hawaii SystemInstituto de Astrofísica de CanariasUniversity of EdinburghSKA ObservatoryEuropean Space Research InstituteInstitució 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 PadovaUniversity of BristolBristol Robotics LaboratoryFractal Systems (Canada)University of OsloJet Propulsion LaboratoryLancaster UniversityFelix ScholarshipDAWN Center for Independent LivingTechnical University of DenmarkInstitut d'Astrophysique de ParisSorbonne UniversitéGoddard Space Flight CenterLaboratoire de Physique ThéoriqueHelsinki Institute of PhysicsCentre de Calcul de l’Institut National de Physique Nucléaire et de Physique des ParticulesUniversité Paris Sciences et LettresUniversity College LondonUniversity of MilanIstituto Nazionale di Fisica Nucleare, Sezione di MilanoFHNW University of Applied Sciences and Arts Northwestern SwitzerlandUniversity of BonnIstituto Nazionale di Fisica Nucleare, Sezione di Roma IUniversité Côte d'AzurObservatoire de la Côte d’AzurInternational University of BeirutÉcole Polytechnique Fédérale de LausanneInstitute for High Energy PhysicsNewcastle UniversityUniversity 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 ChilePark UniversityRoyal 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'AostaAstronomy and SpaceUniversity of OxfordUniversity of SalentoIstituto Nazionale di Fisica Nucleare, Sezione di LecceUniversité Catholique de LilleComputing CenterCase Western Reserve UniversityMax Planck Institute for AstrophysicsTechnical University of MunichSorbonne Paris CitéUniversidad de SalamancaObservatoire astronomique de StrasbourgKavli Institute for the Physics and Mathematics of the UniverseAmes Research CenterBay Area Environmental Research InstituteUniversity of California SystemUniversity of California, IrvineInstituto de Física de CantabriaInstitut de Recherche sur les Lois Fondamentales de l'UniversUniversity of PortsmouthAalto UniversityARC Centre of Excellence for Dark Matter Particle PhysicsSwinburne University of TechnologyUniversity of the Western CapeUniversity of ZurichDurham UniversityStockholm 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 SouthamptonUniversity of CambridgeInstitute of AstronomyFlatiron Health (United States)Flatiron InstituteUniversity of British Columbia
Une affiliation ne permet pas de déduire la nationalité d’un auteur.
Les sujets associés
Astronomy and Astrophysical ResearchHistory and Developments in AstronomySolar and Space Plasma Dynamics