ASTRI data reduction software in the framework of the Cherenkov Telescope Array

Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68378271%3A_____%2F18%3A00552773" target="_blank" >RIV/68378271:_____/18:00552773 - isvavai.cz</a>
Result on the web
<a href="https://doi.org/10.1117/12.2311293" target="_blank" >https://doi.org/10.1117/12.2311293</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1117/12.2311293" target="_blank" >10.1117/12.2311293</a>

Result language
angličtina
Original language name
ASTRI data reduction software in the framework of the Cherenkov Telescope Array
Original language description
The Cherenkov Telescope Array (CTA) is a worldwide project aimed at building the next-generation ground-based gamma-ray observatory. CTA will be composed of two arrays of telescopes of different sizes, one each in the Northern and Southern hemispheres, to achieve full-sky coverage and a ten-fold improvement in sensitivity with respect to the present-generation facilities. Within the CTA project, the Italian National Institute for Astrophysics (INAF) is developing an end-to-end prototype of one of the CTA Small-Size Telescope's designs with a dual-mirror (SST-2M) Schwarzschild-Couder optics design. The prototype, named ASTRI SST-2M, is located at the INAF M.C. Fracastoro observing station in Serra La Nave (Mt. Etna, Sicily) and has started its verification and performance validation phase in fall 2017. nn
Czech name
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Czech description
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Publication year
2018
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

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