Accès ouvert déclaré
2025
article
Euclid Quick Data Release (Q1)
C Laigle, C. Gouin, Florian Sarron, L Quilley, Christophe Pichon, Katarina Kraljic, F. Durret, Nora Elisa Chisari, Ulrike Kuchner, Nicola Malavasi, M. Magliocchetti, H. J. McCracken, Jenny G. Sorce, Y. W. Kang, Conor McPartland, Sune Toft, D. Vibert, N. Aghanim, B. Altieri, A Amara, S. Andreon, N. Auricchio, H. Aussel, C. Baccigalupi, Marco Baldi, A. Balestra, S. Bardelli, Alberto Basset, P Battaglia, Francis Bernardeau, A Biviano, Andrea Bonchi, E. Branchini, M. Brescia, J. Brinchmann, S. Camera, G Cañas-Herrera, V. Capobianco, C. Carbone, J. Carretero, Santiago Casas, M. Castellano, G. Castignani, S. Cavuoti, K. C. Chambers, A Cimatti, C Colodro-Conde, G. Congedo, Christopher J. Conselice, L. Conversi, Y. Copin, F Courbin, H.M Courtois, M. Cropper, A. Da Silva, H. Degaudenzi, S de la Torre, G. De Lucia, A. M. Di Giorgio, C. Dolding, H. Dole, F. Dubath, C. A. J. Duncan, X. Dupac, A. Ealet, S. Escoffier, M. Farina, R. Farinelli, F Faustini, S Ferriol, F. Finelli⋆, S. Fotopoulou, 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, Stephen Gwyn, S. V. H. Haugan, Henk Hoekstra, W. Holmes, I. Hook, F. Hormuth, A. Hornstrup, P. Hudelot, K. Jahnkę, M. Jhabvala, B Joachimi, E. Keihänen, S. Kermiche, A. Kiessling, M. Kilbinger, B. Kubik, 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, E. Medinaceli, S Mei, M Melchior, Y. Mellier, M. Meneghetti, E. Merlin, G. Meylan, A. Mora, M. Moresco, L. Moscardini, Ryota Nakajima, C Neissner, S.-M Niemi, J.W Nightingale, C. Padilla Aranda, S. Paltani, F. Pasian, K. Pedersen, Will J. Percival, V Pettorino, S Pires, G. Polenta, M. Poncet, L. Popa, L. Pozzetti, F. Raison, R. Rébolo, A. Renzi, Jason Rhodes, G. Riccio, E. Romelli, M. Roncarelli, B. Rusholme, R. P. Saglia, Z. Sakr, Ariel G. Sánchez, D. Sapone, B. Sartoris, J.A Schewtschenko, M Schirmer, P. C. Schneider, T. Schrabback, M. Scodeggio, A. Secroun, G. Seidel, M. D. Seiffert, S. Serrano, Patrice Simon, C. Sirignano, G. Sirri, J. Skottfelt, L. Stančo, J Steinwagner, P. Tallada-Crespí, A. N. Taylor, Harry I. Teplitz, I. Tereno, N Tessore, R. Toledo-Moreo, F. Torradeflot, I. Tutusaus, 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, A Cappi, D. Di Ferdinando, J.A. Escartin Vigo, 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, M Viel, M. Wiesmann, Y. Akrami, Sameer Alvi, I.T Andika, S Anselmi, M. Archidiacono, F. Atrio‐Barandela, A. Balaguera-Antolínez, Christophe Benoıst, K. Benson, Daniele Bertacca, M. Béthermin, Alain Blanchard, L Blot, H. Böhringer, S. Borgani, M.L Brown, S Bruton, Anthony Calabro, B. Camacho Quevedo, F Caro, C. S. Carvalho, T. Castro, F Cogato, T. Contini, Asantha Cooray, O. Cucciati, S. Davini, F. De Paolis, G. Desprez, A. Díaz‐Sánchez, J.J Diaz, S. Di Domizio, J. M. Diego, Pierre–Alain Duc, A Enia, Y Fang, A.G Ferrari, P.G Ferreira, A Finoguenov, A. Fontana, A. Franco, K. Ganga, J. García-Bellido, T Gasparetto, V Gautard, E. Gaztañaga, F. Giacomini, F. Gianotti, Anthony H. Gonzalez, G. Gozaliasl, M Guidi, C.M Gutierrez, A Hall, W.G Hartley, C. Hernández-Monteagudo, H. Hildebrandt, J Hjorth, Shahab Joudaki, J. J. E. Kajava, V. Kansal, D Karagiannis, K Kiiveri, C.C Kirkpatrick, Sandor Kruk, J Le Graet, L Legrand, Maria Lembo, Fabio Lepori, G Leroy, G.F Lesci, Julien Lesgourgues, Laura Leuzzi, T.I Liaudat, A. Loureiro, J. F. Macías–Pérez, G. Maggio, E.A Magnier, F. Mannucci, R. Maoli, C. J. A. P. Martins, L. Maurin, M Miluzio, Pierluigi Monaco, A Montoro, Claudio Moretti, G. Morgante, S. Nadathur, Kammila Naidoo, A Navarro-Alsina, Savvas Nesseris, F Passalacqua, K. Paterson, L. Patrizii, A Pisani, D. Potter, S Quai, M. Radovich, P.-F Rocci, S Sacquegna, M Sahlén, D. B. Sanders, E Sarpa, Claudia Scarlata, A. Schneider, M. Schultheis, D Sciotti, Elena Sellentin, Francesco Shankar, L. C. Smith, S. A. Stanford, K Tanidis, 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, D. Scott
2Citations signalées, ce qui n’est pas une note de qualité
189Institutions déclarées
25Pays d’affiliation déclarés
Rattachement africain : fr, au, nl, es, gb, de, it, ch, dk, us, pt, ca, no, fi, lb, ro, cl, at, my, sk, ru, jp, Afrique du Sud, se, uz.
Niveau de preuve : code pays fourni par la source.
Le résumé fourni par la source
Galaxy morphologies and shape orientations are expected to correlate with their large-scale environments, since they grow by accreting matter from the cosmic web and are subject to interactions with other galaxies. We extracted cosmic filaments in projection from the Euclid Quick Data Release 1 (covering 63.1 deg 2 ) at 0.5 < z < 0.9 in tomographic slices of 170 comoving h −1 Mpc using photometric redshifts. Galaxy morphologies are accurately retrieved thanks to the excellent imaging resolution of the visible camera (VIS) of Euclid . The distribution of massive galaxies ( M * > 10 10 M ⊙ ) in the projected cosmic web is analysed as a function of morphology measured from VIS data. Specifically, the 2D alignment of galaxy shapes with large-scale filaments is quantified as a function of Sérsic indices and masses. We find the known trend that more massive galaxies are closer to filament spines. At fixed stellar masses, morphologies correlate both with densities and distances to large-scale filaments. In addition, the large volume of this data set allows us to detect a signal indicating that there is a preferential alignment of the major axis of massive early-type galaxies along projected cosmic filaments. Overall, these results demonstrate our capabilities to carry out detailed studies of galaxy environments with Euclid , which will be extended to higher redshift and lower stellar masses with the future Euclid Deep Survey.
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 UniversitéUniversité Toulouse III - Paul SabatierUniversité Toulouse-I-CapitoleCentre de Biologie du DéveloppementInstitut de Recherche en Informatique de ToulouseUniversité Toulouse - Jean JaurèsInstitut Polytechnique de BordeauxCentre de Biologie Intégrative de ToulouseLyon 1 UniversitéÉcole Normale Supérieure de LyonCentre de Recherche Astrophysique de LyonAstronomy and SpaceObservatoire astronomique de StrasbourgLeiden UniversityUtrecht UniversityInstituto de Física TeóricaUniversity of NottinghamMax Planck Institute for Extraterrestrial PhysicsInstitute for Space Astrophysics and PlanetologyUniversité de LilleUniversité Paris-SaclayInstitut d'Astrophysique SpatialeCentre de Recherche en Informatique, Signal et Automatique de LilleÉcole Centrale de LilleUniversity of GenevaUniversity of CopenhagenDAWN Center for Independent LivingAix-Marseille UniversitéEngineering Science Analysis (United States)University of SurreyBrera Astronomical ObservatoryCommissariat à l'Énergie Atomique et aux Énergies AlternativesAstrophysique, Instrumentation et ModélisationCEA Paris-SaclayOsservatorio di Astrofisica e Scienza dello SpazioUniversité Paris CitéScuola Internazionale Superiore di Studi AvanzatiTrieste Astronomical ObservatoryIstituto Nazionale di Fisica Nucleare, Sezione di TriesteInstitute for Fundamental Physics of the UniverseOsservatorio astronomico di BolognaIstituto Nazionale di Fisica Nucleare, Sezione di BolognaUniversity of BolognaOsservatorio Astronomico di PadovaCentre National d'Études SpatialesInstitut de Physique ThéoriqueEuropean Space AgencyUnited 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 TurinEuropean Space Research and Technology CentreNational Institute for AstrophysicsPort d'Informació CientíficaCentro de Investigaciones Energéticas, Medioambientales y TecnológicasRWTH Aachen UniversityAstronomical Observatory of RomeIstituto Nazionale di Fisica Nucleare, Sezione di NapoliNaples Anesthesia & Physician AssociatesUniversity of Hawaii SystemInstituto de Astrofísica de CanariasRoyal ObservatoryUniversity of EdinburghSKA ObservatoryInstitute of Nuclear Physics of LyonEuropean Space Research InstituteInstitut de Physique des 2 Infinis de LyonInstitució Catalana de Recerca i Estudis AvançatsInstitut Català de Ciències del ClimaLyon CollegeUniversity College LondonUniversity of LisbonLaboratoire d’Astrophysique de MarseilleChâteau GombertCentre de physique des particules de MarseilleUniversity of BristolBristol Robotics LaboratoryLudwig-Maximilians-Universität MünchenFractal Systems (Canada)Herzberg Institute of AstrophysicsUniversity of OsloJet Propulsion LaboratoryLancaster UniversityFelix ScholarshipTechnical University of DenmarkMax Planck Institute for AstronomyGoddard Space Flight CenterLaboratoire de Physique ThéoriqueUniversity of HelsinkiHelsinki Institute of PhysicsCentre de Calcul de l’Institut National de Physique Nucléaire et de Physique des ParticulesJanssen (France)Laboratoire Univers et ThéoriesUniversité Paris Sciences et LettresUniversity 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 ILagrange LaboratoryUniversité Côte d'AzurObservatoire de la Côte d’AzurInternational University of BeirutÉcole Polytechnique Fédérale de LausanneInstitute for High Energy PhysicsNewcastle UniversityUniversity of WaterlooPerimeter InstituteInstitute of Space Science - INFLPR SubsidiaryConsejo Superior de Investigaciones CientíficasUniversidad de La LagunaUnidades Centrales Científico-TécnicasUniversity of PaduaIstituto Nazionale di Fisica Nucleare, Sezione di PadovaInstitut de Recherche en Astrophysique et PlanétologieUniversité Fédérale de Toulouse Midi-PyrénéesUniversity of Saint JosephHeidelberg UniversitySt. Joseph Medical CenterHeidelberg Institute for Theoretical StudiesUniversity of ChileUniversität InnsbruckPark UniversityInstitut d'Estudis Espacials de CatalunyaInstitute of Space SciencesOpen University MalaysiaCalifornia Institute of TechnologyInfrared Processing and Analysis CenterUniversidad Politécnica de CartagenaUniversity of GroningenAstronomical Institute of the Slovak Academy of SciencesUniversity of FerraraIstituto Nazionale di Fisica Nucleare, Sezione di FerraraIstituto di Radioastronomia di BolognaDélégation Paris 7University of OxfordLaboratoire d’Etudes du Rayonnement et de la Matière en Astrophysique et AtmosphèresUniversité 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 UniverseMax Planck Institute for PhysicsUniversity of California, IrvineUniversity of SalentoIstituto Nazionale di Fisica Nucleare, Sezione di LecceInstituto de Física de CantabriaCEA GrenobleCEA CadaracheInstitut de Recherche sur les Lois Fondamentales de l'UniversUniversity of PortsmouthUniversity of FloridaAalto 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 ParticulesLaboratoire de Physique Subatomique et de CosmologieUniversité 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 AstronomyUniversity of OuluFlatiron 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 ResearchScientific Research and Discoveries