Active optics primary mirror support system for the 26m VST telescope
Pietro Schipani, Sergio D’Orsi, Luigi Ferragina, Davide Fierro, Laurent Marty, Cesare Molfese, Francesco Perrotta
Abstract
Pietro Schipani, Sergio D’Orsi, Luigi Ferragina, Davide Fierro, Laurent Marty, Cesare Molfese, Francesco Perrotta
Abstract
The Very Large Telescope Survey Telescope (VST) is equipped with an active optics system in order to correct low-order aberrations. The 2.6 m primary mirror is supported both axially and laterally and is surrounded by several safety devices for earthquake protection. We describe the mirror support system and discuss the results of the qualification test campaign.
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The Very Large Telescope Survey Telescope (VST) is equipped with an active optics system in order to correct low-order aberrations. The 2.6 m primary mirror is supported both axially and laterally and is surrounded by several safety devices for earthquake protection. We describe the mirror support system and discuss the results of the qualification test campaign.
Key concepts: Active optics, Primary mirror, Optics, Telescope, Reflecting telescope, Physics, Axial symmetry, Optical telescope