TROIA adaptive optics system for DAG Telescope

O. Keskin; L. Jolissaint; A. Bouxin; C. Yesilyaprak

doi:10.1117/12.2560528

13 December 2020 TROIA adaptive optics system for DAG Telescope

O. Keskin, L. Jolissaint, A. Bouxin, C. Yesilyaprak

Proceedings Volume 11448, Adaptive Optics Systems VII; 114481P (2020) https://doi.org/10.1117/12.2560528
Event: SPIE Astronomical Telescopes + Instrumentation, 2020, Online Only

Abstract

This paper presents the specifications of TROIA - TuRkish adaptive Optics system for Infrared Astronomy system, the science rationale for these specifications, and description of the site technical and environmental conditions to be taken into account in the adaptive optics (AO) system design for the Eastern Anatolia Observatory - DAG telescope. With it’s 468 actuators, EMCCD camera, and the pyramid wavefront sensor configuration; TROIA is able to adapt the degree of correction to a given guide star (GS) brightness during observations. The high actuator density of TROIA AO system will allow DAG to perform astronomical observations at ExAO performances.

Conference Presentation

Citation Download Citation

O. Keskin, L. Jolissaint, A. Bouxin, and C. Yesilyaprak "TROIA adaptive optics system for DAG Telescope", Proc. SPIE 11448, Adaptive Optics Systems VII, 114481P (13 December 2020); https://doi.org/10.1117/12.2560528

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