Pre-selecting muon events in the camera server of the ASTRI telescopes for the Cherenkov Telescope Array

Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68378271%3A_____%2F16%3A00553675" target="_blank" >RIV/68378271:_____/16:00553675 - isvavai.cz</a>
Result on the web
<a href="https://doi.org/10.1117/12.2230835" target="_blank" >https://doi.org/10.1117/12.2230835</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1117/12.2230835" target="_blank" >10.1117/12.2230835</a>

Result language
angličtina
Original language name
Pre-selecting muon events in the camera server of the ASTRI telescopes for the Cherenkov Telescope Array
Original language description
The Cherenkov Telescope Array (CTA) represents the next generation of ground-based observatories for very high energy gamma-ray astronomy. The CTA will consist of two arrays at two different sites, one in the northern and one in the southern hemisphere. The current CTA design foresees, in the southern site, the installation of many tens of imaging atmospheric Cherenkov telescopes of three different classes, namely large, medium and small, so defined in relation to their mirror area, the northern hemisphere array would consist of few tens of the two larger telescope types. The telescopes will be equipped with cameras composed either of photomultipliers or silicon photomultipliers, and with different trigger and read-out electronics. In such a scenario, several different methods will be used for the telescopes' calibration.n
Czech name
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Czech description
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Publication year
2016
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

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