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AMBER : a near infrared focal instrument for the VLTI

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  • معلومة اضافية
    • Contributors:
      Laboratoire Universitaire d'Astrophysique de Nice (LUAN); Université Nice Sophia Antipolis (1965 - 2019) (UNS)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS); Laboratoire d'Astrophysique de Grenoble (LAOG); Université Joseph Fourier - Grenoble 1 (UJF)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS); INAF - Osservatorio Astrofisico di Arcetri (OAA); Istituto Nazionale di Astrofisica (INAF); Max-Planck-Institut für Radioastronomie (MPIFR); Département Fresnel (FRESNEL); Observatoire de la Côte d'Azur; Université Côte d'Azur (UniCA)-Université Côte d'Azur (UniCA)-Centre National de la Recherche Scientifique (CNRS); ONERA - The French Aerospace Lab Châtillon; ONERA-Université Paris Saclay (COmUE); Division technique INSU/SDU (DTI); Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS); Institut de Recherche en Communications Optiques et Microondes (IRCOM); Université de Limoges (UNILIM)-Centre National de la Recherche Scientifique (CNRS); European Southern Observatory (ESO); Centre de Recherche Astrophysique de Lyon (CRAL); École normale supérieure de Lyon (ENS de Lyon)-Université Claude Bernard Lyon 1 (UCBL); Université de Lyon-Université de Lyon-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)
    • بيانات النشر:
      HAL CCSD
      Académie des sciences (Paris)
    • الموضوع:
      2001
    • Collection:
      ONERA: HAL (Centre français de recherche aérospatiale / French Aerospace Lab)
    • نبذة مختصرة :
      10 pages ; International audience ; AMBER is the General User near-infrared focal instrument of the Very Large Telescope interferometer. Its specifications are based on three key programs on Young Stellar Objects, Active Galactic Nuclei central regions, masses and spectra of hot Extra Solar Planets. It has an imaging capacity because it combines up to three beams and very high accuracy measurement are expected from the spatial filtering of beams by single mode fibers and the comparison of measurements made simultaneously in different spectral channels.
    • Relation:
      info:eu-repo/semantics/altIdentifier/arxiv/astro-ph/0507398; hal-00007570; https://hal.science/hal-00007570; https://hal.science/hal-00007570/document; https://hal.science/hal-00007570/file/cras_ref.pdf; ARXIV: astro-ph/0507398
    • الدخول الالكتروني :
      https://hal.science/hal-00007570
      https://hal.science/hal-00007570/document
      https://hal.science/hal-00007570/file/cras_ref.pdf
    • Rights:
      info:eu-repo/semantics/OpenAccess
    • الرقم المعرف:
      edsbas.1F684830