Paper
10 July 2018 Adaptive optics at the ESO ELT
Author Affiliations +
Abstract
The construction of a diffraction limitable telescope as large as the ESO’s ELT is enabled by its embedded deformable quaternary mirror. Besides its essential function in the telescope control, M4 also contributes to compensating the free atmosphere aberrations for all post-focal AO applications. The paper presents how the telescope manages M4 to maintain its optical performance while offering to the instruments a clean wavefront interface, supporting the desired AO functionalities. The paper reviews the telescope strategy to derive its wavefront dynamic properties directly from the analysis of the control data collected in science mode, with the goal to minimize the observatory time spent on dedicated wavefront calibration tasks.
© (2018) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Henri Bonnet, Fabio Biancat-Marchet, Martin Dimmler, Michael Esselborn, Nick Kornweibel, Miska Le Louarn, Pierre-Yves Madec, Enrico Marchetti, Michael Müller, Sylvain Oberti, Jérôme Paufique, Lorenzo Pettazzi, Babak Sedghi, Jason Spyromilio, Stefan Stroebele, Christophe Vérinaud, and Elise Vernet "Adaptive optics at the ESO ELT", Proc. SPIE 10703, Adaptive Optics Systems VI, 1070310 (10 July 2018); https://doi.org/10.1117/12.2312407
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CITATIONS
Cited by 6 scholarly publications.
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KEYWORDS
Telescopes

Adaptive optics

Wavefronts

Wavefront sensors

Active optics

Segmented mirrors

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