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Optical design of the relay optics for the MICADO SCAO system

Authors :
Zoltan Hubert
Michael Hartl
Mathieu Cohen
Fanny Chemla
Richard Davies
Tristan Buey
Eric Gendron
Yann Clénet
Laboratoire d'études spatiales et d'instrumentation en astrophysique (LESIA)
Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris
Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)
Haute résolution angulaire en astrophysique
Laboratoire d'études spatiales et d'instrumentation en astrophysique = Laboratory of Space Studies and Instrumentation in Astrophysics (LESIA)
Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris
Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris
Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité)
Source :
Proceedings of the SPIE, Adaptive Optics Systems IV, Adaptive Optics Systems IV, Jun 2014, Montréal, Quebec, Canada. pp.33
Publication Year :
2014
Publisher :
SPIE, 2014.

Abstract

We present the current optical design of the Relay Optics (RO) dedicated to the single-conjugate adaptive optics (SCAO) mode for the first light E-ELT imaging camera MICADO. MICADO is a wide-field near-IR camera featuring a 75 arcsec field of view, with spectrographic, astrometric, and coronagraphic capabilities. It has been chosen by ESO as one of the two first-light instruments. MICADO will be optimized for the multi-conjugate adaptive optics module MAORY and will also work in SCAO mode to provide a high-level, on-axis correction (making use of the adaptive secondary M4 in the telescope). For full scientific exploitation and in a phase approach for developing AO performance at the ELT, a SCAO mode is needed for MICADO. It will be a joint development between the MICADO and MAORY consortia and in the long term integrated in MAORY. Different options are presented to accommodate different set of requirements, the development plan of MICADO and MAORY instruments will lead to the final configuration and the used of the SCAO and its RO. They allow Coronagraphic observations providing an intermediate pupil plane to accommodate an atmospheric dispersion corrector and an apodizer.

Details

ISSN :
0277786X
Database :
OpenAIRE
Journal :
SPIE Proceedings
Accession number :
edsair.doi.dedup.....765b5af4ec85b1000fdc528e71d02c5c
Full Text :
https://doi.org/10.1117/12.2056286