<i>Euclid</i> preparation
W. GillardAix-Marseille Université, CNRS/IN2P3, CPPMT. MaciaszekCentre National d’Etudes Spatiales – Centre spatial de ToulouseÉric PrietoAix-Marseille Université, CNRS, CNES, LAMF. GruppMax Planck Institute for Extraterrestrial PhysicsA. CostilleAix-Marseille Université, CNRS, CNES, LAMK. JahnkęMax-Planck-Institut für AstronomieJ. D. ClemensAix-Marseille Université, CNRS/IN2P3, CPPMS DusiniINFN-PadovaM. CarleAix-Marseille Université, CNRS, CNES, LAMC SirignanoDipartimento di Fisica e Astronomia “G. Galilei”, Università di PadovaE. MedinaceliINAF-Osservatorio di Astrofisica e Scienza dello Spazio di BolognaS. LigoriINAF-Osservatorio Astrofisico di TorinoE. FranceschiINAF-Osservatorio di Astrofisica e Scienza dello Spazio di BolognaM. TrifoglioINAF-Osservatorio di Astrofisica e Scienza dello Spazio di BolognaWilliam BonAix-Marseille Université, CNRS, CNES, LAMR. BarbierUniversité Claude Bernard Lyon 1, CNRS/IN2P3, IP2I Lyon, UMR 5822S. FerriolUniversité Claude Bernard Lyon 1, CNRS/IN2P3, IP2I Lyon, UMR 5822A SecrounAix-Marseille Université, CNRS/IN2P3, CPPMN. AuricchioINAF-Osservatorio di Astrofisica e Scienza dello Spazio di BolognaPietro BattagliaINAF-Osservatorio di Astrofisica e Scienza dello Spazio di BolognaC. BonoliINAF-Osservatorio Astronomico di PadovaL. CorcioneINAF-Osservatorio Astrofisico di TorinoF HormuthFelix Hormuth EngineeringD. Le MignantAix-Marseille Université, CNRS, CNES, LAMG. MorganteINAF-Osservatorio di Astrofisica e Scienza dello Spazio di BolognaC. PadillaInstitut de Física d’Altes Energies (IFAE), The Barcelona Institute of Science and TechnologyR. Toledo-MoreoUniversidad Politécnica de Cartagena, Departamento de Electrónica y Tecnología de ComputadorasL. ValenzianoINAF-Osservatorio di Astrofisica e Scienza dello Spazio di BolognaR. BenderMax Planck Institute for Extraterrestrial PhysicsF.J CastanderInstitut d’Estudis Espacials de Catalunya (IEEC), Edifici RDITP. B. LiljeInstitute of Theoretical Astrophysics, University of OsloA. BalestraINAF-Osservatorio Astronomico di PadovaClement BarrièreCEA-Saclay, DRF/IRFU, departement d’ingenierie des systemesMichel BerthéUniversité Paris-Saclay, Université Paris Cité, CEA, CNRS, AIMC. BoderndorfMax Planck Institute for Extraterrestrial PhysicsAnne BonnefoiAix-Marseille Université, CNRS, CNES, LAMV. CapobiancoINAF-Osservatorio Astrofisico di TorinoR. CasasInstitut d’Estudis Espacials de Catalunya (IEEC), Edifici RDITH. S. ChoJet Propulsion Laboratory, California Institute of TechnologyFranck DucretAix-Marseille Université, CNRS, CNES, LAMJean-Luc GimenezAix-Marseille Université, CNRS, CNES, LAMW. HolmesJet Propulsion Laboratory, California Institute of TechnologyA. HornstrupCosmic Dawn Center (DAWN)M. JhabvalaNASA Goddard Space Flight CenterE. JulloAix-Marseille Université, CNRS, CNES, LAMR. KohleyESAC/ESA, Camino Bajo del CastilloB. KubikUniversité Claude Bernard Lyon 1, CNRS/IN2P3, IP2I Lyon, UMR 5822R. LaureijsEuropean Space Agency/ESTECI. LloroSKA Observatory, Jodrell Bank, Lower WithingtonC. MacabiauUniversité Claude Bernard Lyon 1, CNRS/IN2P3, IP2I Lyon, UMR 5822Y. MellierInstitut d’Astrophysique de ParisG PolentaUnited Kingdom Space AgencyG. D. RaccaEuropean Space Agency/ESTECA RenziDipartimento di Fisica e Astronomia “G. Galilei”, Università di PadovaM. SchirmerMax-Planck-Institut für AstronomieG. SeidelMax-Planck-Institut für AstronomieM. SeiffertJet Propulsion Laboratory, California Institute of TechnologyG. SirriINFN-Sezione di BolognaG. SmadjaUniversité Claude Bernard Lyon 1, CNRS/IN2P3, IP2I Lyon, UMR 5822L StancoINFN-PadovaStefanie WachterCarnegie ObservatoriesH AusselUniversité Paris-Saclay, Université Paris Cité, CEA, CNRS, AIMT. AuphanAix-Marseille Université, CNRS/IN2P3, CPPMB. R. GranettINAF-Osservatorio Astronomico di BreraR. CharyInfrared Processing and Analysis Center, California Institute of TechnologyY. CopinUniversité Claude Bernard Lyon 1, CNRS/IN2P3, IP2I Lyon, UMR 5822P. HudelotInstitut d’Astrophysique de Paris, UMR 7095, CNRS, and Sorbonne UniversitéV. Le BrunAix-Marseille Université, CNRS, CNES, LAMF. TorradeflotCentro de Investigaciones Energéticas, Medioambientales y Tecnológicas (CIEMAT)P. N. AppletonP. CasenoveCentre National d’Etudes Spatiales – Centre spatial de ToulousePierre-Yves ChabaudAix-Marseille Université, CNRS, CNES, LAMM FrailisINAF-Osservatorio Astronomico di TriesteM FumanaINAF-IASF MilanoL. GuzzoDipartimento di Fisica “Aldo Pontremoli”, Università degli Studi di MilanoG. MainettiCentre de Calcul de l’IN2P3/CNRSD. MainoDipartimento di Fisica “Aldo Pontremoli”, Università degli Studi di MilanoM. MorescoDipartimento di Fisica e Astronomia “Augusto Righi” – Alma Mater Studiorum Università di BolognaWill J. PercivalDepartment of Physics and Astronomy, University of WaterlooR. ScaramellaINAF-Osservatorio Astronomico di RomaM. ScodeggioINAF-IASF MilanoNathaniel R. StickleyCalifornia Institute of TechnologyD. VibertAix-Marseille Université, CNRS, CNES, LAMY. WangInfrared Processing and Analysis Center, California Institute of TechnologyJ. ZoubianAix-Marseille Université, CNRS/IN2P3, CPPMN. AghanimUniversité Paris-Saclay, CNRS, Institut d’astrophysique spatialeB. AltieriESAC/ESA, Camino Bajo del CastilloA. AmaraSchool of Mathematics and Physics, University of SurreyS. AndreonINAF-Osservatorio Astronomico di BreraC BaccigalupiIFPU, Institute for Fundamental Physics of the UniverseMarco BaldiDipartimento di Fisica e Astronomia, Università di BolognaS BardelliINAF-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. BresciaDepartment of Physics “E. Pancini”, University Federico IIJ. BrinchmannFaculdade de Ciências da Universidade do Porto, Rua do Campo de AlegreS. CameraDipartimento di Fisica, Università degli Studi di TorinoG Cañas-HerreraEuropean Space Agency/ESTECC. CarboneINAF-IASF Milano
ABI
Аннотация
ESA’s Euclid cosmology mission relies on the very sensitive and accurately calibrated spectroscopy channel of the Near-Infrared Spectrometer and Photometer (NISP). With three operational grisms in two wavelength intervals, NISP provides diffraction-limited slitless spectroscopy over a field of 0.57 deg 2 . A blue grism, BG E , covers the wavelength range 926–1366 nm at a spectral resolution (ℛ) of 440–900 for a 0.″5 diameter source with a dispersion of 1.24 nm px −1 . Two red grisms, RG E , span 1206 to 1892 nm at ℛ = 550–740 and a dispersion of 1.37 nm px −1 . We describe the construction of the grisms as well as the ground testing of the flight model of the NISP instrument, where these properties were established.
Темы
Идентификаторы
Цитирования и источники
Цитирований: 0Использованных источников: 14
Показатели — AkademScholar · Скоро