Paper
2 September 2016 MCAO with LINC-NIRVANA at LBT: preparing for first light
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Abstract
LINC-NIRVANA is an innovative, high-resolution, near-infrared imager for the Large Binocular Telescope. Its Multi-Conjugate Adaptive Optics system uses natural guide-stars and the layer-oriented, multiple-field of view approach for high sky coverage and eventual interferometric beam combination. We describe LINC-NIRVANA’s particular flavour of MCAO and its associated challenges, and report on final lab integration and system level testing. LINC-NIRVANA is currently at the telescope undergoing final alignment and tests before First Light late this fall.
© (2016) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
T. M. Herbst, C. Arcidiacono, T. Bertram, P. Bizenberger, F. Briegel, R. Hofferbert, M. Kürster, and R. Ragazzoni "MCAO with LINC-NIRVANA at LBT: preparing for first light", Proc. SPIE 9909, Adaptive Optics Systems V, 99092U (2 September 2016); https://doi.org/10.1117/12.2232596
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Cited by 4 scholarly publications.
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KEYWORDS
Stars

Adaptive optics

Telescopes

Turbulence

Mirrors

Wavefront sensors

Actuators

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