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

Kód výsledku v 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>

Výsledek na webu

<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>

Jazyk výsledku

angličtina

Název v původním jazyce

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

Popis výsledku v původním jazyce

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

Název v anglickém jazyce

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

Popis výsledku anglicky

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

Druh

D - Stať ve sborníku

CEP obor

—

OECD FORD obor

10303 - Particles and field physics

Projekt

—

Návaznosti

—

Rok uplatnění

2016

Kód důvěrnosti údajů

S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Název statě ve sborníku

Proceedings of SPIE

ISBN

9781510602052

ISSN

0277-786X

e-ISSN

1996-756X

Počet stran výsledku

10

Strana od-do

1-10

Název nakladatele

SPIE

Místo vydání

Bellingham

Místo konání akce

Edinburgh

Datum konání akce

26. 6. 2016

Typ akce podle státní příslušnosti

WRD - Celosvětová akce

Kód UT WoS článku

000388804600079