Accès ouvert déclaré
2026
preprint
Euclid Quick Data Release (Q1). The Strong Lensing Discovery Engine F -- Bright and low-redshift strong lenses
Euclid Collaboration, L. R. Ecker, M. Fabricius, S. Seitz, R. Saglia, N. E. P. Lines, Paul H. Holloway, Tian Li, A. Verma, F. Balzer, Qiutong Jin, A. Manjón-García, S. H. Vincken, J. Wilde, J. A. Acevedo Barroso, J. W. Nightingale, K. Rojas, S. Schuldt, M. Walmsley, T. E. Collett, G. Despali, Alessandro Sonnenfeld, C. Tortora, R. B. Metcalf, R. Bender, C. Saulder, Elisabeth Baeten, Claude Cornen, D. Delley, Kyle Finner, A. Galan, R. Gavazzi, L. C. Johnson, L. Leuzzi, Christine Macmillan, P. J. Marshall, M. Millon, A. More, L. A. Moustakas, James F. Pearson, J. -N. Pippert, C. Scarlata, Dominique Sluse, C. Spiniello, T. T. Thai, L. Ulivi, H. Wang, Xiaopeng Xu, F. Courbin, M. Meneghetti, N. Aghanim, B. Altieri, S. Andreon, N. Auricchio, C. Baccigalupi, M. Baldi, A. Balestra, S. Bardelli, P. Battaglia, A. Biviano, E. Branchini, M. Brescia, S. Camera, G. Cañas-Herrera, V. Capobianco, C. Carbone, J. Carretero, S. Casas, M. Castellano, G. Castignani, S. Cavuoti, K. C. Chambers, A. Cimatti, C Colodro-Conde, G. Congedo, C. J. Conselice, L. Conversi, Y. Copin, A. Costille, H. M. Courtois, Maureen Cropper, A. Da Silva, Hubert Degaudenzi, G. De Lucia, C. Dolding, H. Dole, F. Dubath, Xavier Dupac, S. Dusini, A. Ealet, S. Escoffier, Marcelo Farina, R. Farinelli, F Faustini, S. Ferriol, Francesco Finelli, P. Fosalba, S. Fotopoulou, M. Frailis, E. Franceschi, M. Fumana, S. Galeotta, K. George, W. Gillard, B. Gillis, C. Giocoli, P Gómez-Álvarez, J. Gracia-Carpio, A. Grazian, F. Grupp, L. Guzzo, S. V. H. Haugan, H. Hoekstra, Warren Holmes, F. Hormuth, A. Hornstrup, K. Jahnke, M. Jhabvala, B. Joachimi, E. Keihänen, Smain Kermiche, A. Kiessling, B. Kubik, M. Kümmel, Martina Kunz, Hannu Kurki-Suonio, A. M. C. Le Brun, D. Le Mignant, 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. J. Massey, E. Medinaceli, S. Mei, Y. Mellier, E. Merlin, G. Meylan, A. Mora, M. Moresco, L. Moscardini, R. Nakajima, Christian Neissner, R. C. Nichol, S. -M. Niemi, C. Padilla, S. Paltani, F. Pasian, K. Pedersen, W. J. Percival, V. Pettorino, S. Pires, G. Polenta, M. Poncet, L. Pozzetti, F. Raison, A. Renzi, J. Rhodes, G. Riccio, H. -W. Rix, E. Romelli, M. Roncarelli, E. Rossetti, Z. Sakr, A. G. Sánchez, D. Sapone, B. Sartoris, P. Schneider, T. Schrabback, A. Secroun, G. Seidel, S. Serrano, P. Simon, C. Sirignano, G. Sirri, L. Stanco, J. Steinwagner, P. Tallada-Crespí, A. N. Taylor, H. I. Teplitz, I. Tereno, N Tessore, S. Toft, R. Toledo-Moreo, F. Torradeflot, I. Tutusaus, L. Valenziano, J. Väliviita, T. Vassallo, Y. Wang, J. Weller, A. Zacchei, G. Zamorani, F. M. Zerbi, E. Zucca, M. Ballardini, M. Bolzonella, E. Bozzo, C. Burigana, R. Cabanac, A. Cappi, T. Castro, B. Clément, J. A. Escartin Vigo, L. Gabarra, J. García-Bellido, V Gautard, S. Hemmati, M. Huertas-Company, J. Macias-Perez, R. Maoli, J Martín-Fleitas, M. Maturi, N. Mauri, P. Monaco, A Pezzotta, M. Pöntinen, C. Porciani, I Risso, V Scottez, M. Sereno, M. Tenti, M. Tucci, M. Viel, M. Wiesmann, Y. Akrami, I. T. Andika, G. Angora, S. Anselmi, Maria Archidiacono, F. Atrio-Barandela, L. Bazzanini, P. Bergamini, D. Bertacca, M. Bethermin, Florian Beutler, A. Blanchard, L. Blot, M. Bonici, S. Borgani, M. L. Brown, S. Bruton, A. Calabro, B. Camacho Quevedo, F. Caro, C. S. Carvalho, Y. Charles, F. Cogato, S. Conseil, A. R. Cooray, O. Cucciati, S. Davini, F. De Paolis, G. Desprez, A. Díaz-Sánchez, S. Di Domizio, J. M. Diego, P. -A. Duc, Véronique Duret, M. Y. Elkhashab, A Enia, Y. Fang, A. Finoguenov, A. Fontana, A. Franco, K. Ganga, T Gasparetto, E. Gaztanaga, F. Giacomini, Fluvio Gianotti, G. Gozaliasl, A. Gruppuso, M. Guidi, C. M. Gutierrez, A. Hall, H. Hildebrandt, J. Hjorth, L. K. Hunt, J. J. E. Kajava, Y. Kang, V. Kansal, D. Karagiannis, K. Kiiveri, J. Kim, C. C. Kirkpatrick, S. Kruk, M. Lattanzi, L. Legrand, F. Lepori, G. Leroy, G. F. Lesci, J. Lesgourgues, T. I. Liaudat, A. Loureiro, M. Magliocchetti, F. Mannucci, C. J. A. P. Martins, L. Maurin, M Miluzio, C. Moretti, G. Morgante, K. Naidoo, P. Natoli, A. Navarro-Alsina, S. Nesseris, D. Paoletti, Francesca Passalacqua, K. Paterson, L. Patrizii, A. Pisani, Douglas Potter, G. W. Pratt, S Quai, M. Radovich, G. Rodighiero, W. Roster, S Sacquegna, M Sahlén, D. B. Sanders, E. Sarpa, A. Schneider, D. Sciotti, E. Sellentin, L. C. Smith, J. G. Sorce, K. Tanidis, C. Tao, F. Tarsitano, G. Testera, Romain Teyssier, S. Tosi, A. Troja, A. Venhola, D. Vergani, G. Vernardos, G. Verza, P Vielzeuf, S. Vinciguerra, N. A. Walton, A. H. Wright
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176Institutions déclarées
25Pays d’affiliation déclarés
Rattachement africain : de, gb, es, ch, us, fr, it, ca, cn, jp, in, be, nl, pt, ro, no, dk, fi, lb, cl, at, sk, au, Afrique du Sud, se.
Niveau de preuve : code pays fourni par la source.
Le résumé fourni par la source
We present 72 additional galaxy-galaxy strong lenses that complement the sample discovered in the Euclid Quick Release 1 data (63.1 deg^2) of the Strong Lens Discovery Engine (SLDE) papers A-E. It is shown that previous pre-selection of potential lenses, which excluded objects from the Gaia catalogue, led to missing several bright and low-redshift strong lenses, adding more than 10% new strong lens candidates compared to the previous search. In total, the catalogue includes 38 "grade A" (confident) and 34 "grade B" (probable) candidates. These lenses are identified through a combination of two independent searches for bright nearby objects: one based on machine-learning models followed by expert visual inspection, and the other based solely on expert visual inspection, targeting objects not included in the initial machine-learning selection (a limitation identified only after extensive visual inspection). With these additional strong lens candidates, we augment the expected number of high-confidence candidates in the Euclid Wide Survey from previous forecasts to 120000. Detailed semi-automated lens modelling confirms at least 41 systems out of 72, a fraction consistent with that found in SLDE A (315 out of 488). These include: multiple edge-on disc lenses; sources with arcs near the lens centre; "red sources"; and an edge-on disk galaxy lensing a galaxy merger, producing two sets of lensed features, an Einstein ring and a doubly imaged component. The median redshift of these systems is $Δ$ z ~ 0.3 lower than that of the SLDE A sample.
Ce résumé expose les affirmations des auteurs. BNTIC ne l’interprète pas comme une validation indépendante des résultats.
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Les institutions déclarées
Max Planck Institute for Extraterrestrial PhysicsLudwig-Maximilians-Universität MünchenUniversity of PortsmouthUniversity of OxfordUniversidad Politécnica de CartagenaFHNW University of Applied Sciences and Arts Northwestern SwitzerlandInstitut Català de Ciències del ClimaInstitut de Ciències del CosmosJet Propulsion LaboratoryUniversité Bourgogne Franche-ComtéÉcole Polytechnique Fédérale de LausanneNewcastle UniversityUniversity of MilanNational Institute for AstrophysicsUniversity of ManchesterCanadian Institute for Theoretical AstrophysicsIstituto Nazionale di Fisica Nucleare, Sezione di BolognaOsservatorio di Astrofisica e Scienza dello SpazioUniversity of BolognaShanghai Jiao Tong UniversityShanghai Astronomical ObservatoryAstronomical Observatory of CapodimonteCalifornia Institute of TechnologyInfrared Processing and Analysis CenterMax Planck Institute for AstrophysicsTechnical University of MunichCentre National de la Recherche ScientifiqueAix-Marseille UniversitéInstitut d'Astrophysique de ParisSorbonne UniversitéSLAC National Accelerator LaboratoryKavli Institute for Particle Astrophysics and CosmologyUniversity of GenevaKavli Institute for the Physics and Mathematics of the UniverseInter-University Centre for Astronomy and AstrophysicsThe Open UniversityUniversity of MinnesotaUniversity of LiègeEuropean Southern ObservatoryNational Astronomical Observatory of JapanArcetri Astrophysical ObservatoryCentro de AstrobiologíaUniversity of Southern CaliforniaStatewide California Earthquake CenterUniversity of California, IrvineInstitució Catalana de Recerca i Estudis AvançatsInstitute of Space SciencesUniversité Paris-SaclayInstitut d'Astrophysique SpatialeEuropean Space Astronomy CentreBrera Astronomical ObservatoryScuola Internazionale Superiore di Studi AvanzatiUniversity of TriesteTrieste Astronomical ObservatoryIstituto Nazionale di Fisica Nucleare, Sezione di TriesteInstitute for Fundamental Physics of the UniverseOsservatorio Astronomico di PadovaIstituto Nazionale di Fisica Nucleare, Sezione di GenovaUniversity of GenoaIstituto Nazionale di Fisica Nucleare, Sezione di TorinoOsservatorio Astrofisico di TorinoUniversity of TurinLeiden UniversityRoyal ObservatoryUniversity of EdinburghPort d'Informació CientíficaCentro de Investigaciones Energéticas, Medioambientales y TecnológicasDeutsches Zentrum für Luft- und Raumfahrt e. V. (DLR)Astronomical Observatory of RomeIstituto Nazionale di Fisica Nucleare, Sezione di NapoliUniversity of Hawaii SystemInstituto de Astrofísica de CanariasEuropean Space Research InstituteLyon 1 UniversitéInstitut National de Physique Nucléaire et de Physique des ParticulesInstitut de Physique des 2 Infinis de LyonUniversity College LondonUniversity of LisbonInstitute of Astrophysics and Space SciencesIstituto Nazionale di Fisica Nucleare, Sezione di PadovaCentre de physique des particules de MarseilleInstitute for Space Astrophysics and PlanetologyAgenzia Spaziale ItalianaInstitut d'Estudis Espacials de CatalunyaInstitute of Space Science - INFLPR SubsidiaryUniversity of BristolLMU KlinikumTécnicas Reunidas (Spain)Istituto Nazionale di Fisica Nucleare, Sezione di MilanoUniversity of OsloDAWN Center for Independent LivingTechnical University of DenmarkMax Planck Institute for AstronomyGoddard Space Flight CenterHelsinki Institute of PhysicsUniversity of HelsinkiLaboratoire Univers et ThéoriesSKA ObservatoryCentre de Calcul de l’Institut National de Physique Nucléaire et de Physique des ParticulesUniversity of BonnIstituto Nazionale di Fisica Nucleare, Sezione di Roma IDurham UniversityUniversité Paris CitéEuropean Space AgencyInstitute for High Energy PhysicsUniversity of SurreyEuropean Space Research and Technology CentreUniversity of CopenhagenUniversity of WaterlooPerimeter InstituteCommissariat à l'Énergie Atomique et aux Énergies AlternativesAstrophysique, Instrumentation et ModélisationCEA Paris-SaclayCentre National d'Études SpatialesUniversity of PaduaSaint Joseph UniversityHeidelberg UniversityInstitut de Recherche en Astrophysique et PlanétologieHeidelberg Institute for Theoretical StudiesUniversity of ChileUniversität InnsbruckUniversity of FerraraIstituto Nazionale di Fisica Nucleare, Sezione di FerraraIstituto di Radioastronomia di BolognaUniversité Côte d'AzurObservatoire de la Côte d’AzurInstitute for High Performance Computing and NetworkingConsejo Superior de Investigaciones CientíficasUniversidad Autónoma de MadridInstitut de Recherche sur les Lois Fondamentales de l'UniversUniversité Paris Sciences et LettresSorbonne Paris CitéLaboratoire d’Etudes du Rayonnement et de la Matière en Astrophysique et AtmosphèresInstitut polytechnique de GrenobleUniversité Grenoble AlpesSapienza University of RomeUniversité Catholique de LilleCase Western Reserve UniversityUniversidad de SalamancaObservatoire astronomique de StrasbourgUniversité de StrasbourgKavli Institute for the Physics and Mathematics of the UniverseUniversity of SalentoIstituto Nazionale di Fisica Nucleare, Sezione di LecceUniversity of GroningenInstituto de Física de CantabriaAalto UniversityUniversidad de La LagunaAstronomical Institute of the Slovak Academy of SciencesRuhr University BochumUniversity of TurkuTurku Centre for Computer ScienceSerco (United Kingdom)ARC Centre of Excellence for Dark Matter Particle PhysicsSwinburne University of TechnologyUniversity of the Western CapeUniversity of CambridgeUniversity of ZurichStockholm UniversityImperial College LondonUniversidade do PortoCentro de Astrofísica da Universidade do PortoCollurania Teramo ObservatoryUppsala UniversityUniversité de LilleCentre de Recherche en Informatique, Signal et Automatique de LilleÉcole Centrale de LilleETH ZurichPrinceton UniversityUniversity of OuluAmerican Museum of Natural HistoryLehman CollegeThe Abdus Salam International Centre for Theoretical Physics (ICTP)International Centre for Theoretical SciencesFlatiron Health (United States)Flatiron Institute
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