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Accès ouvert déclaré 2026 article

Euclid Quick Data Release (Q1)

2Citations signalées, ce qui n’est pas une note de qualité
171Institutions déclarées
25Pays d’affiliation déclarés

Rattachement africain : fr, lb, it, gb, in, be, nl, sk, us, pt, es, de, ch, ca, no, dk, fi, ro, cl, ru, jp, au, Afrique du Sud, se, uz. Niveau de preuve : code pays fourni par la source.

Le résumé fourni par la source

The extent to which the environment affects galaxy evolution has been under scrutiny by researchers for decades. With the first data from Euclid , we can begin to systematically study a wide range of environments and their effects as a function of redshift, using 63 deg 2 of space-based data. In this paper, we present results from the Euclid Quick Data Release, where we measured the passive-density and morphology-density relations in the redshift range z = 0.25–1. We determined if a galaxy is passive using the specific star formation rate, and we classified the morphologies of galaxies using the Sérsic index n and the u − r colours. We measured the local environmental density of each galaxy using the N th-nearest neighbour method. We find that at a fixed stellar mass, the quenched fraction (the fraction of galaxies that have ceased star formation) increases with increasing local environmental density up to z = 1. This result is indicative of the separability of the effects from the stellar mass and the environment. Similarly, at all redshifts in this work, the early-type galaxy fraction increases with increasing density at fixed stellar mass, meaning the environment also transforms the morphology of the galaxy independently of stellar mass, up to M * ≲ 10 10.8 M ⊙ . For M * ≳ 10 10.8 M ⊙ , almost all galaxies are early-types, with minimal impact from the environment. At z > 0.75, the morphology depends mostly on stellar mass, with only low-mass galaxies being affected by the environment. Given that the morphology classifications use u − r colours, these are correlated to the star formation rate, and as such our morphology results should be taken with caution, yet future morphology classifications should help verify these results. To summarise, we successfully identify the passive-density and morphology-density relations at 0.25 < z < 1. Future Euclid data releases are key to confirm these trends at higher redshifts.

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, mais le titre doit être comparé manuellement.

Titre Crossref
<i>Euclid</i> Quick Data Release (Q1)
Date Crossref
01/07/2026
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 ScientifiqueUniversité Paris CitéInternational University of BeirutTrieste Astronomical ObservatoryInstitute for Fundamental Physics of the UniverseUniversity of SouthamptonInter-University Centre for Astronomy and AstrophysicsUniversity of PortsmouthInstitute for Space Astrophysics and PlanetologyUniversité Paris-SaclayInstitut d'Astrophysique SpatialeCentre de Recherche en Informatique, Signal et Automatique de LilleÉcole Centrale de LilleGhent UniversityUniversity of GroningenAstronomical Institute of the Slovak Academy of SciencesCardiff UniversityAstronomical Observatory of CapodimonteEngineering Science Analysis (United States)University of SurreyBrera Astronomical ObservatoryOsservatorio di Astrofisica e Scienza dello SpazioCommissariat à l'Énergie Atomique et aux Énergies AlternativesAstrophysique, Instrumentation et ModélisationCEA Paris-SaclayScuola 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 PadovaEuropean Space AgencyUnited Kingdom Space AgencyOsservatorio Astrofisico di TorinoIstituto Nazionale di Fisica Nucleare, Sezione di GenovaUniversity of GenoaFederico II University HospitalUniversidade do PortoInstitute of Astrophysics and Space SciencesIstituto Nazionale di Fisica Nucleare, Sezione di TorinoUniversity of TurinLeiden UniversityEuropean Space Research and Technology CentreNational Institute for AstrophysicsPort d'Informació CientíficaCentro de Investigaciones Energéticas, Medioambientales y TecnológicasRWTH Aachen UniversityInstitut d'Estudis Espacials de CatalunyaInstitute of Space SciencesAstronomical 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 UniversitéInstitute of Nuclear Physics of LyonInstitut de Physique des 2 Infinis de LyonInstitució Catalana de Recerca i Estudis AvançatsInstitut Català de Ciències del ClimaLyon CollegeUniversity College LondonUniversity of LisbonUniversity of GenevaAix-Marseille UniversitéCentre de physique des particules de MarseilleUniversity of BristolBristol Robotics LaboratoryLudwig-Maximilians-Universität MünchenMax Planck Institute for Extraterrestrial PhysicsHerzberg Institute of AstrophysicsUniversity of OsloJet Propulsion LaboratoryFelix ScholarshipDAWN Center for Independent LivingTechnical University of DenmarkInstitut d'Astrophysique de ParisSorbonne UniversitéMax 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 ParticulesUniversité Paris Sciences et LettresLaboratoire d’Astrophysique de MarseilleChâteau GombertUniversity 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'AzurLagrange LaboratoryObservatoire de la Côte d’AzurÉcole Polytechnique Fédérale de LausanneInstitute for High Energy PhysicsNewcastle UniversityUniversity of CopenhagenUniversity of WaterlooPerimeter InstituteCentre National d'Études SpatialesInstitute of Space Science - INFLPR SubsidiaryConsejo Superior de Investigaciones CientíficasUniversidad de La LagunaUnidades Centrales Científico-TécnicasUniversity of PaduaIstituto Nazionale di Fisica Nucleare, Sezione di PadovaUniversité 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 UniversityCalifornia Institute of TechnologyInfrared Processing and Analysis CenterUniversidad Politécnica de CartagenaUniversity of FerraraIstituto Nazionale di Fisica Nucleare, Sezione di FerraraIstituto di Radioastronomia di BolognaUniversity of OxfordUniversité Catholique de LilleUniversité de LilleComputing CenterCase Western Reserve UniversityMax Planck Institute for AstrophysicsTechnical University of MunichJanssen (France)Laboratoire Univers et ThéoriesSorbonne Paris CitéUniversidad de SalamancaObservatoire astronomique de StrasbourgKavli 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'UniversAstronomy and SpaceAalto 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 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

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