Phase A AO system design and performance for MOSAIC at the ELT - Archive ouverte HAL
Communication Dans Un Congrès Année : 2018

Phase A AO system design and performance for MOSAIC at the ELT

Timothy Morris
  • Fonction : Auteur
Kjetil Dohlen
David Jenkins
  • Fonction : Auteur
Simon Morris
  • Fonction : Auteur
Edward Younger
  • Fonction : Auteur

Résumé

MOSAIC is a mixed-mode multiple object spectrograph planned for the ELT that uses a tiled focal plane to support a variety of observing modes. The MOSAIC AO system uses 4 LGS WFS and up to 4 NGS WFS positioned anywhere within the full 10 arcminute ELT field of view to control either the ELT M4/5 alone for GLAO operation feeding up to 200 targets in the focal plane, or M4/5 in conjunction with 10 open-loop DMs for MOAO correction. In this paper we present the overall design and performance of the MOSAIC GLAO and MOAO systems.

Dates et versions

hal-02409306 , version 1 (13-12-2019)

Identifiants

Citer

Timothy Morris, Alastair Basden, Ariadna Calcines-Rosario, Kjetil Dohlen, Cornelis Dubbeldam, et al.. Phase A AO system design and performance for MOSAIC at the ELT. SPIE Astronomical Telescopes + Instrumentation, 2018, Jun 2018, Austin, United States. ⟨10.1117/12.2313562⟩. ⟨hal-02409306⟩
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