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Proceedings Paper

Calibration strategy and optics for ARGOS at the LBT
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Paper Abstract

Effective calibration procedures play an important role for the efficiency and performance of astronomical instrumentation. We report on the calibration scheme for ARGOS, the Laser Guide Star (LGS) facility at the LBT. An artificial light source is used to feign the real laser beacons and perform extensive testing of the system, independent of the time of day and weather conditions, thereby greatly enhancing the time available for engineering. Fibre optics and computer generated holograms (CGHs) are used to generate the necessary wavefront. We present the optomechanical design, and discuss the expected accuracy, as well as tolerances in assembly and alignment.

Paper Details

Date Published: 14 July 2010
PDF: 5 pages
Proc. SPIE 7736, Adaptive Optics Systems II, 773630 (14 July 2010); doi: 10.1117/12.857231
Show Author Affiliations
Christian Schwab, Univ. of Heidelberg (Germany)
Diethard Peter, Max-Planck-Institut für Astronomie (Germany)
Simon Aigner, Dioptic GmbH (Germany)


Published in SPIE Proceedings Vol. 7736:
Adaptive Optics Systems II
Brent L. Ellerbroek; Michael Hart; Norbert Hubin; Peter L. Wizinowich, Editor(s)

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