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Pushing high angular resolution and high contrast observations on the VLTI from Y to L band with the Asgard instrumental suite: integration status and plans

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  • معلومة اضافية
    • بيانات النشر:
      International Society for Optical Engineering, 2024.
    • الموضوع:
      2024
    • نبذة مختصرة :
      editorial reviewed
      ESO’s Very Large Telescope Interferometer has a history of record-breaking discoveries in astrophysics and significant advances in instrumentation. The next leap forward is its new visitor instrument, called Asgard. It comprises four natively collaborating instruments: HEIMDALLR, an instrument performing both fringe tracking and stellar interferometry simultaneously with the same optics, operating in the K band; Baldr, a Strehl optimizerin the H band; BIFROST, a spectroscopic combiner to study the formation processes and properties of stellar and planetary systems in the Y-J-H bands; and NOTT, a nulling interferometer dedicated to imaging nearby young planetary systems in the L band. The suite is in its integration phase in Europe and should be shipped to Paranal in 2025. In this article, we present details of the alignment and calibration unit, the observing
      Asgard
    • Relation:
      info:eu-repo/grantAgreement/EC/H2020/101004719; info:eu-repo/grantAgreement/EC/H2020/101004719; info:eu-repo/grantAgreement/EC/H2020/101004719; urn:issn:0277-786X; urn:issn:1996-756X
    • الرقم المعرف:
      10.1117/12.3016296
    • Rights:
      open access
      http://purl.org/coar/access_right/c_abf2
      info:eu-repo/semantics/openAccess
    • الرقم المعرف:
      edsorb.321638