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ASTRI SST-2M: the design evolution from the prototype to the array telescope
- Source :
- Ground-based and Airborne Telescopes VII.
- Publication Year :
- 2018
- Publisher :
- SPIE, 2018.
-
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.
- Subjects :
- Design evolution
segmented optics
High energy
Computer science
Astrophysics::High Energy Astrophysical Phenomena
Imaging atmospheric Cherenkov telescopes
law.invention
Telescope
Observatory
law
Angular resolution
Silicon compounds
Design enhancement
Very high energies
Airborne telescopes
Silicon compounds, Angular resolution
Cherenkov telescope arrays
Schwarzschild
Segmented optics
Very high energies, Gamma rays
CTA
Gamma rays
Schwarzschild-Couder
Small Size Telescope
Cherenkov radiation
Remote sensing
Astrophysics::Instrumentation and Methods for Astrophysics
Cherenkov Telescope Array
Focus (optics)
Subjects
Details
- Database :
- OpenAIRE
- Journal :
- Ground-based and Airborne Telescopes VII
- Accession number :
- edsair.doi.dedup.....c95aceab5303045f0240c3166a2a4cbe