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  5. Models for the active optics system of the ASTRI SST-2M prototype proposed for the Cherenkov Telescope Array
 

Models for the active optics system of the ASTRI SST-2M prototype proposed for the Cherenkov Telescope Array

Date Issued
2016
Author(s)
GARDIOL, Daniele  
•
GIRO, Enrico  
•
LESSIO, Luigi  
•
LOREGGIA, Davide  
•
RODEGHIERO, Gabriele  
•
RUSSO, Federico  
DOI
10.1117/12.2214548
Abstract
ASTRI SST-2M is an end-to-end prototype of Small Size class of Telescope proposed for the Cherenkov Telescope Array (CTA). Currently under completion at the Serra La Nave observing station (Mt. Etna, Catania, Italy), the ASTRI SST- 2M telescope is the first imaging dual-mirror telescope ever realized for Cherenkov telescopes. A mini-array of nine such telescopes will form the ASTRI mini-array proposed as a precursor and initial seed of CTA to be installed at the final CTA southern site. ASTRI SST-2M is equipped with an active optics system, controlling both the segmented primary mirror and the monolithic secondary mirror, which allows optical re-alignment during telescope slew. We describe the hardware and software solution that have been implemented for optics control and the models we developed for the system.
Coverage
Integrated Modeling of Complex Optomechanical Systems II
All editors
Riva, Marco
Series
PROCEEDINGS OF SPIE  
Volume
10012
Start page
1001207-1
Conferenece
Integrated Modeling of Complex Optomechanical Systems II
Conferenece place
Varenna, Italy
Conferenece date
7-9 October, 2015
Uri
http://hdl.handle.net/20.500.12386/24405
Url
https://www.spiedigitallibrary.org/conference-proceedings-of-spie/10012/1/Models-for-the-active-optics-system-of-the-ASTRI-SST/10.1117/12.2214548.short
Issn Identifier
0277-786X
Ads BibCode
2016SPIE10012E..07G
Rights
open.access
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