51. The design of an adaptive optics telescope: the case of DAG
- Author
-
Gregory P. Lousberg, Laurent Jolissaint, Lorenzo Zago, Cahit Yeşilyaprak, Onur Keskin, Sinan Kaan Yerli, Emeric Mudry, Işık Üniversitesi, Mühendislik Fakültesi, Makine Mühendisliği Bölümü, Işık University, Faculty of Engineering, Department of Mechanical Engineering, Keskin, Onur, Hall, HJ, Gilmozzi, R, Marshall, HK, Bölüm Yok, Yerli, Sinan Kaan -- 0000-0001-9717-5349, Yesilyaprak, Cahit -- 0000-0002-9481-2848, and [Jolissaint, Laurent -- Zago, Lorenzo] Univ Appl Sci Western Switzerland, Yverdon, Switzerland -- [Keskin, Onur] FMV Isik Univ, Fac Engn, Dept Mech Engn, Istanbul, Turkey -- [Yerli, Sinan Kaan] Orta Dogu Tekn Univ METU, Dept Phys, Ankara, Turkey -- [Yesilyaprak, Cahit] Ataturk Univ, Astrophys Res & Applicat Ctr ATASAM, Erzurum, Turkey -- [Yesilyaprak, Cahit] Ataturk Univ, Fac Sci, Dept Astron & Astrophys, Erzurum, Turkey -- [Mudry, Emeric -- Lousberg, Gregory] AMOS, Rue Chasseurs Ardennais 2, B-4031 Angleur, Belgium -- European Ind Engn Srl, Via Torino 151-A, I-30172 Mestre Venezia, Italy
- Subjects
Ritchey-Chretien telescope ,Reflecting telescope ,Zernike polynomials ,Design optimization ,DAG observatory ,Potential impacts ,Astrophysics ,01 natural sciences ,Space telescopes ,Static aberrations ,law.invention ,adaptive optics ,010309 optics ,Telescope ,Active optics ,symbols.namesake ,Optics ,Focal lengths ,law ,0103 physical sciences ,Focal length ,Ritchey-chretien telescope ,Adaptive optics ,010303 astronomy & astrophysics ,Zernike modes ,Physics ,Design decisions ,business.industry ,Optical design ,First light ,Ritchey–Chrétien telescope ,symbols ,Airborne telescopes ,business ,active optics ,Telescopes - Abstract
Conference on Ground-Based and Airborne Telescopes VI -- JUN 26-JUL 01, 2016 -- Edinburgh, SCOTLAND WOS: 000387731100107 In this paper, we describe in detail the optical design of DAG, a new 4 m telescope for Turkey. DAG is an "adaptive optics friendly" telescope, in a sense that each design decision is taken considering the potential impact on the AO performance (vibrations, static aberrations etc.) The objective is to make this telescope fully ready for AO at first light. It is designed as a Ritchey-Chretien combination, 56 m focal length, with Nasmyth foci only, and active optics. Its total RMS error is expected to be 45 nm up to Zernike mode 78, and 26 nm for the higher, non AO corrected modes. A final design optimization has been done by the telescope manufacturers, demonstrating that our AO-based requirements can be satisfied, without much difficulty. SPIE
- Published
- 2016