PROCEEDINGS ARTICLE | July 27, 2016
Proc. SPIE. 9906, Ground-based and Airborne Telescopes VI
KEYWORDS: Monochromatic aberrations, Telescopes, Telescopes, Mirrors, Sensors, Error analysis, Wavefronts, Adaptive optics, Space telescopes, Optical instrument design, Active optics
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-Chrétien 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.
