ASTRI SST-2M: the design evolution from the prototype to the array telescope

Date Issued
2018
Author(s)
Marchiori, G.
•
Busatta, A.
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Marcuzzi, E.
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Manfrin, C.
•
Folla, I.
•
•
•
•
•
Tosti, G.
•
Antolini, E.
•
•
DOI
Abstract
The Cherenkov Telescope Array (CTA) observatory will represent the new frontier of imaging atmospheric Cherenkov Telescope. The simultaneous use of large, medium and small telescopes (respectively LST, MST and SST) will allow to explore the astronomy related to the very high energy domain, typical of Gamma rays, with a sensitivity, angular resolution and image quality never seen before. Within this project, ASTRI, the Italian 2 mirrors Schwarzshild-Couder configuration Small SST led by Italian National Institute of Astronomy (INAF), has moved quickly developing a 4m class telescope prototype which has been tested with results which demonstrates excellent performance as well as wide margins for further improvements. On the basis of the experiences made on the prototype, this paper focus on the design enhancements carried out for the telescope which will be part of the Cherenkov Telescope Array.
Coverage
Ground-based and Airborne Telescopes VII
All editors
Marshall, Heather K.; Spyromilio, Jason
Series
Volume
10700
Start page
107005W
Conferenece
Ground-based and Airborne Telescopes VII
Conferenece place
Austin, Texas, United States
Conferenece date
10-15 June, 2018
Uri
Url
Issn Identifier
0277-786X
Ads BibCode
2018SPIE10700E..5WM
Rights
open.access
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