Paper
28 July 2010 Testing the VLT AO facility with ASSIST
Remko Stuik, Robin Arsenault, Wilfried Boland, Atul Deep, Bernard Delabre, Norbert Hubin, Johann Kolb, Paolo La Penna, Frank Molster, Emiel Wiegers
Author Affiliations +
Abstract
The testing and verification of ESO Very Large Telescope Adaptive Optics Facility (VLT-AOF) requires new and innovative techniques to deal with the absence of an intermediate focus on the telescope. ASSIST, The Adaptive Secondary Setup and Instrument STimulator, was developed to provide a testing facility for the ESO AOF and will allow off-telescope testing of three elements of the VLT Adaptive Optics Facility; the Deformable Secondary Mirror (DSM) and the AO systems for MUSE and HAWK-I (GALACSI and GRAAL). ASSIST will provide a full testing environment which includes an interferometric testing mode for the DSM, an on-axis testing mode with a single wavefront sensor and full operation testing modes for both the AO systems. Both natural as well as laser guide stars will be simulated under various asterisms and a realistic turbulent atmosphere will be provided for varying atmospheric conditions. ASSIST passed its final design review and is now being manufactured, integrated and tested and will be operational in mid 2011, in time for first testing with the DSM.
© (2010) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Remko Stuik, Robin Arsenault, Wilfried Boland, Atul Deep, Bernard Delabre, Norbert Hubin, Johann Kolb, Paolo La Penna, Frank Molster, and Emiel Wiegers "Testing the VLT AO facility with ASSIST", Proc. SPIE 7736, Adaptive Optics Systems II, 77363M (28 July 2010); https://doi.org/10.1117/12.857791
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KEYWORDS
Adaptive optics

Mirrors

Stars

Manufacturing

Turbulence

Telescopes

Beam splitters

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