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Euclid Quick Data Release (Q1)

W. RosterMax Planck Institute for Extraterrestrial PhysicsM. SalvatoMax Planck Institute for Extraterrestrial PhysicsJohannes BüchnerMax Planck Institute for Extraterrestrial PhysicsR. ShirleyMax Planck Institute for Extraterrestrial PhysicsElisabeta LussoINAF-Osservatorio Astrofisico di ArcetriHermine LandtDepartment of Physics, Centre for Extragalactic Astronomy, Durham UniversityG. ZamoraniINAF-Osservatorio di Astrofisica e Scienza dello Spazio di BolognaM. SiudekInstituto de Astrofísica de Canarias (IAC), Departamento de Astrofísica, Universidad de La Laguna (ULL)Brivael LalouxINAF-Osservatorio Astronomico di CapodimonteT. Matamoro ZatarainSchool of Physics, HH Wills Physics Laboratory, University of BristolF. RicciINAF-Osservatorio Astronomico di RomaS. FotopoulouSchool of Physics, HH Wills Physics Laboratory, University of BristolAnna Ferré-MateuUniversidad de La Laguna, Departamento de AstrofísicaX. Lopez LopezINAF-Osservatorio di Astrofisica e Scienza dello Spazio di BolognaN. AghanimInstitut d'Astrophysique SpatialeB. AltieriESAC/ESAأ هــانـى محمــد عمارةSchool of Mathematics and Physics, University of SurreyS. AndreonINAF-Osservatorio Astronomico di BreraN. AuricchioINAF-Osservatorio di Astrofisica e Scienza dello Spazio di BolognaH. AusselUniversité Paris-Saclay, Université Paris Cité, CEA, CNRS, AIMC. BaccigalupiINAF-Osservatorio Astronomico di TriesteMarco BaldiINAF-Osservatorio di Astrofisica e Scienza dello Spazio di BolognaA. BalestraINAF-Osservatorio Astronomico di PadovaS. BardelliINAF-Osservatorio di Astrofisica e Scienza dello Spazio di BolognaP. BattagliaINAF-Osservatorio di Astrofisica e Scienza dello Spazio di BolognaA. BivianoIFPU, Institute for Fundamental Physics of the UniverseA BonchiSpace Science Data Center, Italian Space AgencyE. BranchiniDipartimento di Fisica, Università di GenovaM. BresciaINAF-Osservatorio Astronomico di CapodimonteJ BrinchmannInstituto de Astrofísica e Ciências do Espaço, Universidade do Porto, CAUPS. CameraDipartimento di Fisica, Università degli Studi di TorinoG Cañas-HerreraLeiden Observatory, Leiden UniversityV. CapobiancoINAF-Osservatorio Astrofisico di TorinoC. CarboneINAF-IASF MilanoJ. CarreteroPort d’Informació Científica, Campus UABS. CasasInstitute for Theoretical Particle Physics and Cosmology (TTK), RWTH Aachen UniversityM. CastellanoNational Institute for AstrophysicsG. CastignaniINAF-Osservatorio di Astrofisica e Scienza dello Spazio di BolognaS. CavuotiNaples Anesthesia & Physician AssociatesK. C. ChambersInstitute for Astronomy, University of HawaiiA. CimattiDipartimento di Fisica e Astronomia “Augusto Righi” – Alma Mater Studiorum Università di BolognaC. Colodro-CondeInstituto de Astrofísica de CanariasG. CongedoInstitute for Astronomy, University of Edinburgh, Royal ObservatoryChristopher J. ConseliceJodrell Bank Centre for Astrophysics, Department of Physics and Astronomy, University of ManchesterL. ConversiESA - Agence Spatiale Européenne = European Space Agency (Agence spatiale européenne (ESA) 8-10, rue Mario Nikis F-75015 Paris - France)Y. CopinUniversité Claude Bernard Lyon 1, CNRS/IN2P3, IP2I Lyon, UMR 5822F. CourbinInstitució Catalana de Recerca i Estudis Avançats (ICREA)H. M. CourtoisInstitute of Nuclear Physics of LyonM. CropperMullard Space Science Laboratory, University College LondonA. Da SilvaDepartamento de Física, Faculdade de Ciências, Universidade de LisboaH. DegaudenziDepartment of Astronomy, University of GenevaG. De LuciaINAF-Osservatorio Astronomico di TriesteA. M. Di GiorgioINAF-Istituto di Astrofisica e Planetologia SpazialiC. DoldingMullard Space Science Laboratory, University College LondonH. DoleInstitut d'Astrophysique SpatialeF. DubathDepartment of Astronomy, University of GenevaC. A. J. DuncanJodrell Bank Centre for Astrophysics, Department of Physics and Astronomy, University of ManchesterX. DupacESAC/ESAS. DusiniINFN-PadovaS. EscoffierAix-Marseille Université, CNRS/IN2P3, CPPMMaximilian FabriciusUniversitäts-Sternwarte München, Fakultät für Physik, Ludwig-Maximilians-Universität MünchenM. FarinaINAF-Istituto di Astrofisica e Planetologia SpazialiR. FarinelliINAF-Osservatorio di Astrofisica e Scienza dello Spazio di BolognaF. FaustiniNational Institute for AstrophysicsS. FerriolUniversité Claude Bernard Lyon 1, CNRS/IN2P3, IP2I Lyon, UMR 5822F. Finelli⋆INAF-Osservatorio di Astrofisica e Scienza dello Spazio di BolognaP FosalbaInstitut d’Estudis Espacials de Catalunya (IEEC)N. FourmanoitAix-Marseille Université, CNRS/IN2P3, CPPMM. FrailisINAF-Osservatorio Astronomico di TriesteE. FranceschiINAF-Osservatorio di Astrofisica e Scienza dello Spazio di BolognaS. GaleottaINAF-Osservatorio Astronomico di TriesteKoshy GeorgeUniversitäts-Sternwarte München, Fakultät für Physik, Ludwig-Maximilians-Universität MünchenB. GillisUniversity of EdinburghC. GiocoliINAF-Osservatorio di Astrofisica e Scienza dello Spazio di BolognaJ Gracia-CarpioMax Planck Institute for Extraterrestrial PhysicsB. R. GranettINAF-Osservatorio Astronomico di BreraA. GrazianINAF-Osservatorio Astronomico di PadovaF. GruppMax Planck Institute for Extraterrestrial PhysicsStephen GwynHerzberg Astronomy and Astrophysics Research CentreS. V. H. HauganInstitute of Theoretical Astrophysics, University of OsloW. HolmesJet Propulsion Laboratory, California Institute of TechnologyI. HookDepartment of Physics, Lancaster UniversityF. HormuthFelix Hormuth EngineeringA. HornstrupCosmic Dawn Center (DAWN)P. (P) HudelotIAP - Institut d'Astrophysique de Paris (98bis, bd Arago - 75014 Paris France - France)K. JahnkęMax-Planck-Institut für AstronomieM JhabvalaNASA Goddard Space Flight CenterE. KeihänenS. KermicheAix-Marseille Université, CNRS/IN2P3, CPPMA. KiesslingJet Propulsion Laboratory, California Institute of TechnologyB. KubikInstitut de Physique des 2 Infinis de LyonM KümmelUniversitäts-Sternwarte München, Fakultät für Physik, Ludwig-Maximilians-Universität MünchenM. KunzLaboratoire de Physique ThéoriqueH. Kurki‐SuonioDepartment of PhysicsQ Le Boulc'HCentre de Calcul de l’IN2P3/CNRSA. M. C. Le BrunLaboratoire d’etude de l’Univers et des phenomenes eXtremes, Observatoire de Paris, Université PSL, Sorbonne Université, CNRSD. Le MignantAix-Marseille Université, CNRS, CNES, LAMS. LigoriINAF-Osservatorio Astrofisico di TorinoP. B. LiljeInstitute of Theoretical Astrophysics, University of OsloV. LindholmDepartment of Physics
2025en
ABI

Annotatsiya

To better understand the role of active galactic nuclei (AGN) in galaxy evolution, it is crucial to work with a complete and pure AGN sample. X-ray surveys are key to doing so, but their larger positional uncertainties complicate counterpart (CTP) association, further compounded by the limited availability of deep, uniform multi-wavelength ancillary data. Euclid is revolutionising this identification effort, offering extensive coverage of nearly the entire extragalactic sky, particularly in the near-infrared bands, where AGN are more easily detected. Using the first Euclid Quick Data Release (Q1), we validated the methods for identifying and classifying Euclid CTPs of known point-like sources from major X-ray surveys, including XMM- Newton , Chandra , and eROSITA. Using Bayesian statistics, combined with machine learning (ML), as incorporated in the algorithm NWAY , we identified the CTPs of 11 286 X-ray sources from the three X-ray telescopes. For the large majority of 10 194 sources, the association is unique, with the remaining ∼10% of multi-CTP cases equally split between XMM- Newton and eROSITA. Six percent of the Euclid CTPs are detected in more than one X-ray survey. We then used ML to distinguish between Galactic (8%) and extragalactic (92%) sources. We computed photo- z s using deep learning for the 9259 sources detected in the tenth data release of the DESI Legacy Survey, reaching an accuracy and a fraction of outliers of roughly 5%. Based on their X-ray luminosities, all CTPs identified as extragalactic are classified as AGN, most of which appear as type I AGN according to their hardness ratios. With this paper, we release our catalogue, which includes identifiers, basic X-ray properties, the reliability of the associations, and additional property extensions, such as Galactic- or extragalactic classifications and photometric/spectroscopic redshifts. We also provide probabilities for sub-selecting the sample based on purity and completeness, in order to allow users to tailor the sample according to their specific needs.

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