Accès ouvert déclaré
2026
article
Euclid Quick Data Release (Q1)
C. Gouin, C. Laigle, F. Sarron, T. Bonnaire, J. G. Sorce, N. Aghanim, M. Magliocchetti, L. Quilley, P. Boldrini, F. Durret, C. Pichon, U. Kuchner, N. Malavasi, K. Kraljic, R. Gavazzi, Y. Kang, S. A. Stanford, P. Awad, B. Altieri, A. Amara, S. Andreon, N Auricchio, H. Aussel, C Baccigalupi, M. Baldi, A. Balestra, S. Bardelli, A. Basset, P. Battaglia, F Bernardeau, A Biviano, A. Bonchi, E Branchini, M Brescia, J. Brinchmann, S Camera, G. Cañas-Herrera, V. Capobianco, C. Carbone, J. Carretero, 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, 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. Fabricius, M. Farina, F. Faustini, S. Ferriol, F Finelli, S. Fotopoulou, M. Frailis, E. Franceschi, S. Galeotta, K George, B. Gillis, C. Giocoli, P. Gómez-Alvarez, J Gracia-Carpio, B. R. Granett, A. Grazian, F. Grupp, S. Gwyn, S. V. H. Haugan, W. L. Holmes, I. M. Hook, F. Hormuth, A Hornstrup, P. Hudelot, K. Jahnke, M. Jhabvala, B. Joachimi, E Keihänen, S. Kermiche, A. Kiessling, M. Kilbinger, B. Kubik, M. Kümmel, M Kunz, H Kurki-Suonio, O. Lahav, 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. J. Massey, S. Maurogordato, H. J. McCracken, E Medinaceli, S Mei, Y. Mellier, M. Meneghetti, E. Merlin, G. Meylan, A Mora, M. Moresco, L. Moscardini, R. Nakajima, C. Neissner, S.-M. Niemi, J. W. Nightingale, C. Padilla, S. Paltani, F. Pasian, J. A. Peacock, K. Pedersen, W. J. Percival, V. Pettorino, S. Pires, G. Polenta, M. Poncet, L. A. Popa, L. Pozzetti, F. Raison, R. Rebolo, A. Renzi, J. Rhodes, G. Riccio, E Romelli, M. Roncarelli, B. Rusholme, R. Saglia, Z. Sakr, A. G. Sánchez, D Sapone, B. Sartoris, J. A. Schewtschenko, M. Schirmer, P. Schneider, T Schrabback, M. Scodeggio, A Secroun, G. Seidel, S. Serrano, P Simon, C. Sirignano, G. Sirri, J. Skottfelt, L. Stanco, J Steinwagner, P. Tallada-Crespí, D Tavagnacco, A. N. Taylor, H. I. Teplitz, I. Tereno, N. Tessore, S. Toft, R. Toledo-Moreo, F Torradeflot, A. Tsyganov, I. Tutusaus, L. Valenziano, J Valiviita, T. Vassallo, G. Verdoes Kleijn, A. Veropalumbo, Y. D. Wang, J. Weller, A. Zacchei, G. Zamorani, F. M. Zerbi, 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, M. Maturi, 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, S Alvi, I. T. Andika, S. Anselmi, M. Archidiacono, F. Atrio-Barandela, A. Balaguera-Antolinez, C. Benoist, K. Benson, P. Bergamini, D. Bertacca, M. Bethermin, A. Blanchard, L Blot, H. Böhringer, M. L. Brown, S. Bruton, A Calabro, B Camacho Quevedo, F. Caro, C. S. Carvalho, T Castro, F. Cogato, A. R. Cooray, O. Cucciati, S. Davini, F. De Paolis, G. Desprez, A. Díaz-Sánchez, J. Casanueva Diaz, S. Di Domizio, J. M. Diego, P.-A. Duc, A. Enia, Y. Q. Fang, A. G. Ferrari, P. G. Ferreira, A. Finoguenov, A. Fontana, A. Franco, K. Ganga, J. García-Bellido, T. Gasparetto, V. Gautard, E. Gaztanaga, F Giacomini, F. Gianotti, G. Gozaliasl, M. Guidi, C. M. Gutierrez, A Hall, W. G. Hartley, S Hemmati, C. Hernández-Monteagudo, H. Hildebrandt, J. Hjorth, J. J. E. Kajava, V. Kansal, D. Karagiannis, K Kiiveri, C. C. Kirkpatrick, S Kruk, J. Le Graet, L. Legrand, M Lembo, F. Lepori, G. Leroy, G. F. Lesci, J. Lesgourgues, L. Leuzzi, T. I. Liaudat, A. Loureiro, J. Macias-Perez, G. Maggio, E. A. Magnier, F. Mannucci, R. Maoli, C. J. A. P. Martins, L. Maurin, M. Migliaccio, M. Miluzio, P. Monaco, A Montoro, C. Moretti, G. Morgante, S Nadathur, K. Naidoo, A. Navarro-Alsina, S. Nesseris, F. Passalacqua, K. Paterson, L. Patrizii, A. Pisani, D Potter, S. Quai, M. Radovich, S Sacquegna, M. Sahlén, D. B. Sanders, E. Sarpa, A. Schneider, D. Sciotti, D. Scognamiglio, E. Sellentin, F. Shankar, L. C. Smith, K. Tanidis, G. Testera, R. Teyssier, S. Tosi, A. Troja, M Tucci, C. Valieri, A Venhola, D. Vergani, G Verza, P Vielzeuf, N. A. Walton, D. Scott
1Citations signalées, ce qui n’est pas une note de qualité
176Institutions déclarées
27Pays d’affiliation déclarés
Rattachement africain : fr, it, Algérie, kr, au, gb, de, ch, nl, us, pt, es, in, ca, no, dk, fi, lb, ro, cl, at, sk, ru, jp, Afrique du Sud, se, uz.
Niveau de preuve : code pays fourni par la source.
Le résumé fourni par la source
The matter around galaxy clusters is distributed over several filaments, reflecting their positions as nodes in the large-scale cosmic web. The number of filaments connected to a cluster, i.e. its connectivity, is expected to affect the physical properties of clusters. Using the first Euclid galaxy catalogue from the Euclid Quick Release 1 (Q1), we investigated the connectivity of galaxy clusters and how it correlates with their physical and galaxy member properties. Around 220 clusters located within the three fields of Q1 (covering ∼63 deg 2 ) were analysed in the redshift range 0.2 < z < 0.7. Due to the photometric redshift uncertainty, we reconstructed the cosmic web skeleton, and measured the cluster connectivity, in 2D projected slices with a thickness of 170 comoving h −1 Mpc and centred on each cluster redshift, by using two different filament finder algorithms on the most massive galaxies ( M ★ > 10 10.3 M ⊙ ). In agreement with previous measurements, we recovered the mass-connectivity relation independently of the filament detection algorithm, showing that the most massive clusters are, on average, connected to a larger number of cosmic filaments, consistent with hierarchical structure formation models. Furthermore, we explored the possible correlations between connectivities and two cluster properties: the fraction of early-type galaxies and the Sérsic index of galaxy members. Our result suggests that the clusters populated by early-type galaxies exhibit higher connectivity compared to clusters dominated by late-type galaxies. These preliminary investigations highlight our ability to quantify the impact of the cosmic web’s connectivity on cluster properties with Euclid .
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 ToulouseÉcole Normale Supérieure - PSLLaboratoire de Physique de l'Ecole Normale SupérieureUniversité Paris-SaclayInstitut d'Astrophysique SpatialeCentre de Recherche en Informatique, Signal et Automatique de LilleÉcole Centrale de LilleInstitute for Space Astrophysics and PlanetologyLyon 1 UniversitéCentre de Recherche Astrophysique de LyonCentre de Recherche en Astronomie Astrophysique et GéophysiqueUniversité Paris Sciences et LettresObservatoire de ParisKyung Hee UniversityAstronomy and SpaceUniversity of NottinghamMax Planck Institute for Extraterrestrial PhysicsObservatoire astronomique de StrasbourgAix-Marseille UniversitéUniversity of GenevaLeiden UniversityEngineering Science Analysis (United States)University of SurreyBrera Astronomical ObservatoryOsservatorio di Astrofisica e Scienza dello SpazioUniversité Paris CitéCommissariat à l'Énergie Atomique et aux Énergies AlternativesAstrophysique, Instrumentation et ModélisationCEA Paris-SaclayScuola 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 TecnológicasAstronomical Observatory of RomeIstituto Nazionale di Fisica Nucleare, Sezione di NapoliNaples Anesthesia & Physician AssociatesUniversity of Hawaii SystemInstituto de Astrofísica de CanariasRoyal ObservatoryUK Astronomy Technology CentreSKA ObservatoryEuropean Space Research InstituteInstitut de Physique des 2 Infinis de LyonInstitució Catalana de Recerca i Estudis AvançatsInstitut Català de Ciències del ClimaLyon CollegeDepartment of SpaceUniversity College LondonUniversity of LisbonCentre de physique des particules de MarseilleLudwig-Maximilians-Universität MünchenUniversity of BristolBristol Robotics LaboratoryFractal Systems (Canada)Herzberg Institute of AstrophysicsUniversity of OsloJet Propulsion LaboratoryLancaster UniversityFelix ScholarshipDAWN Center for Independent LivingTechnical University of DenmarkMax Planck Institute for AstronomyGoddard Space Flight CenterLaboratoire de Physique ThéoriqueHelsinki Institute of PhysicsCentre de Calcul de l’Institut National de Physique Nucléaire et de Physique des ParticulesUniversity 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 IObservatoire 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 PaduaIstituto Nazionale di Fisica Nucleare, Sezione di PadovaUniversité Fédérale de Toulouse Midi-PyrénéesUniversity of Saint JosephHeidelberg UniversitySt. Joseph Medical CenterInstitut de Recherche en Astrophysique et PlanétologieHeidelberg Institute for Theoretical StudiesUniversity of ChileUniversität InnsbruckPark UniversityInstitut d'Estudis Espacials de CatalunyaInstitute of Space SciencesThe Open UniversityCalifornia 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 BolognaUniversity of OxfordUniversité Catholique de LilleComputing CenterInstituto de Física de CantabriaCase 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 LecceInstitut 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 UniversityRWTH Aachen 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 PortoUniversity of Rome Tor VergataPrinceton UniversityCentre for Theoretical Physics and AstrophysicsMathematical 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
Galaxies: Formation, Evolution, PhenomenaAstronomy and Astrophysical ResearchAstrophysics and Star Formation Studies