2010Applied OpticsRequires access

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

Open publisher page 38 citations

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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What this paper is about

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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OpenAlex reports 38 citations for this work. Citation counts describe recorded attention and do not establish research quality.

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Available 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.

Key concepts: Active optics, Primary mirror, Optics, Telescope, Reflecting telescope, Physics, Axial symmetry, Optical telescope

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