The active optics system of the VLT Survey Telescope (VST) adopts a positioning system for the secondary mirror, a system to support and modify the shape of the 2.6-m primary mirror, and a Shack-Hartmann wavefront sensor. This paper describes the concepts of the VST active optics and the commissioning of the whole system on the ESO's Paranal Observatory. 2012 SPIE.
Schipani P., Magrin D., Noethe L., Arcidiacono C., Argomedo J., Dall'Ora M., et al. (2012). The active optics system of the VST: Concepts and results. 1000 20TH ST, PO BOX 10, BELLINGHAM, WA 98227-0010 USA : SPIE-INT SOC OPTICAL ENGINEERING [10.1117/12.925493].
The active optics system of the VST: Concepts and results
Umbriaco G.
2012
Abstract
The active optics system of the VLT Survey Telescope (VST) adopts a positioning system for the secondary mirror, a system to support and modify the shape of the 2.6-m primary mirror, and a Shack-Hartmann wavefront sensor. This paper describes the concepts of the VST active optics and the commissioning of the whole system on the ESO's Paranal Observatory. 2012 SPIE.File in questo prodotto:
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