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Euclid preparation. Overview of Euclid infrared detector performance from ground tests

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162Institutions déclarées
23Pays d’affiliation déclarés

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

Le résumé fourni par la source

The paper describes the objectives, design and findings of the pre-launch ground characterisation campaigns of the Euclid infrared detectors. The pixel properties, including baseline, bad pixels, quantum efficiency, inter pixel capacitance, quantum efficiency, dark current, readout noise, conversion gain, response nonlinearity, and image persistence were measured and characterised for each pixel. We describe in detail the test flow definition that allows us to derive the pixel properties and we present the data acquisition and data quality check software implemented for this purpose. We also outline the measurement protocols of all the pixel properties presented and we provide a comprehensive overview of the performance of the Euclid infrared detectors as derived after tuning the operating parameters of the detectors. The main conclusion of this work is that the performance of the infrared detectors Euclid meets the requirements. Pixels classified as non-functioning accounted for less than 0.2% of all science pixels. IPC coupling is minimal and crosstalk between adjacent pixels is less than 1% between adjacent pixels. 95% of the pixels show a QE greater than 80% across the entire spectral range of the Euclid mission. The conversion gain is approximately 0.52 ADU/e-, with a variation less than 1% between channels of the same detector. The reset noise is approximately equal to 23 ADU after reference pixels correction. The readout noise of a single frame is approximately 13 $e^-$ while the signal estimator noise is measured at 7 $e^-$ in photometric mode and 9 $e^-$ in spectroscopic acquisition mode. The deviation from linear response at signal levels up to 80 k$e^-$ is less than 5% for 95% of the pixels. Median persistence amplitudes are less than 0.3% of the signal, though persistence exhibits significant spatial variation and differences between detectors.

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Les institutions déclarées

Institute of Nuclear Physics of LyonInstitut de Physique des 2 Infinis de LyonLyon 1 UniversitéCentre National de la Recherche ScientifiqueInstitut National de Physique Nucléaire et de Physique des ParticulesCentre de physique des particules de MarseilleAix-Marseille UniversitéEuropean Space AgencyEuropean Space Astronomy CentreEuropean Space Research and Technology CentreCentre National d'Études SpatialesEuropean Space Research InstituteJet Propulsion LaboratoryUniversité Bourgogne Franche-ComtéGoddard Space Flight CenterCarnegie ObservatoriesMax Planck Institute for AstronomyMax Planck Institute for Extraterrestrial PhysicsLudwig-Maximilians-Universität MünchenOsservatorio Astronomico di PadovaOsservatorio Astrofisico di TorinoIstituto Nazionale di Fisica Nucleare, Sezione di PadovaOsservatorio di Astrofisica e Scienza dello SpazioUniversity of GroningenLeiden UniversityLaboratoire d’Astrophysique de MarseilleChâteau GombertIstituto Nazionale di Fisica Nucleare, Sezione di BolognaUniversity of BolognaUniversity of PaduaUniversidad Politécnica de CartagenaInstitut d'Astrophysique SpatialeUniversité Paris-SaclayBrera Astronomical ObservatoryScuola Internazionale Superiore di Studi AvanzatiUniversity of TriesteTrieste Astronomical ObservatoryIstituto Nazionale di Fisica Nucleare, Sezione di TriesteInstitute for Fundamental Physics of the UniverseCommissariat à l'Énergie Atomique et aux Énergies AlternativesInstitut d'Astrophysique de ParisCEA Paris-SaclayInstitut de Physique ThéoriqueSorbonne UniversitéAgenzia Spaziale ItalianaIstituto Nazionale di Fisica Nucleare, Sezione di GenovaUniversity of GenoaAstronomical Observatory of CapodimonteUniversidade do PortoInstitute of Astrophysics and Space SciencesIstituto Nazionale di Fisica Nucleare, Sezione di TorinoUniversity of TurinNational Institute for AstrophysicsPort d'Informació CientíficaCentro de Investigaciones Energéticas, Medioambientales y TecnológicasInstitute of Space SciencesInstitut d'Estudis Espacials de CatalunyaInstitute of Space Science - INFLPR SubsidiaryAstronomical Observatory of RomeIstituto Nazionale di Fisica Nucleare, Sezione di NapoliUniversity of Hawaii SystemInstituto de Astrofísica de CanariasRoyal ObservatoryUniversity of EdinburghUniversity of ManchesterInstitució Catalana de Recerca i Estudis AvançatsInstitut Català de Ciències del ClimaInstitut de Ciències del CosmosUniversity of LisbonUniversity of GenevaInstitute for Space Astrophysics and PlanetologyUniversity of BristolUniversity of MilanIstituto Nazionale di Fisica Nucleare, Sezione di MilanoUniversity of OsloLancaster UniversityDAWN Center for Independent LivingTechnical University of DenmarkUniversity of HelsinkiHelsinki Institute of PhysicsCentre de Calcul de l’Institut National de Physique Nucléaire et de Physique des ParticulesObservatoire de ParisLaboratoire Univers et ThéoriesUniversity College LondonSKA ObservatoryFHNW University of Applied Sciences and Arts Northwestern SwitzerlandUniversity of BonnIstituto Nazionale di Fisica Nucleare, Sezione di Roma IDurham UniversityLagrange LaboratoryUniversité Côte d'AzurObservatoire de la Côte d’AzurUniversité Paris CitéÉcole Polytechnique Fédérale de LausanneCalifornia Institute of TechnologyInstitute for High Energy PhysicsUniversity of SurreyUniversity of CopenhagenUniversity of WaterlooPerimeter InstituteAstrophysique, Instrumentation et ModélisationConsejo Superior de Investigaciones CientíficasUniversidad de La LagunaUnidades Centrales Científico-TécnicasInstitut de Recherche en Astrophysique et PlanétologieSaint Joseph UniversityHeidelberg UniversityHeidelberg Institute for Theoretical StudiesUniversity of ChileUniversität InnsbruckInfrared Processing and Analysis CenterUniversity of FerraraIstituto Nazionale di Fisica Nucleare, Sezione di FerraraIstituto di Radioastronomia di BolognaUniversity of OxfordUniversité de LilleUniversité Catholique de LilleInstitute for High Performance Computing and NetworkingCase Western Reserve UniversityUniversidad Autónoma de MadridJanssen (France)Max Planck Institute for AstrophysicsTechnical University of MunichUniversité Paris Sciences et LettresUniversidad de SalamancaObservatoire astronomique de StrasbourgUniversité de StrasbourgKavli Institute for the Physics and Mathematics of the UniverseUniversity of California, Los AngelesUniversity of California, IrvineUniversity of SalentoIstituto Nazionale di Fisica Nucleare, Sezione di LecceInstituto de Física de CantabriaValongo ObservatoryCEA GrenobleCEA CadaracheInstitut de Recherche sur les Lois Fondamentales de l'UniversUniversity of PortsmouthAalto UniversityAstronomical Institute of the Slovak Academy of SciencesRuhr University BochumUniversity of TurkuSerco (United Kingdom)ARC Centre of Excellence for Dark Matter Particle PhysicsSwinburne University of TechnologyUniversity of the Western CapeUniversity of CambridgeUniversity of ZurichStockholm UniversityLaboratoire de Physique Subatomique et de CosmologieImperial College LondonInstitut polytechnique de GrenobleUniversité Grenoble AlpesArcetri Astrophysical ObservatorySapienza University of RomeCentro de Astrofísica da Universidade do PortoUppsala UniversityPrinceton UniversityUniversity of OuluFlatiron Health (United States)Flatiron InstituteUniversity of Massachusetts Amherst

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Les sujets associés

Calibration and Measurement TechniquesInfrared Target Detection Methodologies

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