Development of a SiPM based camera for Cherenkov Telescope Array
Identifikátory výsledku
Kód výsledku v IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68378271%3A_____%2F17%3A00553313" target="_blank" >RIV/68378271:_____/17:00553313 - isvavai.cz</a>
Výsledek na webu
<a href="https://doi.org/10.1016/j.nuclphysbps.2017.06.013" target="_blank" >https://doi.org/10.1016/j.nuclphysbps.2017.06.013</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1016/j.nuclphysbps.2017.06.013" target="_blank" >10.1016/j.nuclphysbps.2017.06.013</a>
Alternativní jazyky
Jazyk výsledku
angličtina
Název v původním jazyce
Development of a SiPM based camera for Cherenkov Telescope Array
Popis výsledku v původním jazyce
The Italian Institute of Nuclear Physics (INFN) is involved in the development of a prototype for a SiPM-based camera for the Cherenkov Telescope Array (CTA), a new generation of telescopes for ground - based gamma ray astronomy. In this framework, an R&D program for the development of SiPMs suitable for Cherenkov light detection (Near-Ultraviolet SiPMs) has been carried out. The developed device is a High Density NUV-SiPM based on a micro cell of 30 mu m x 30 mu m and 6 mm x 6 mm area produced by Fondazione Bruno Kessler (FBK). A full characterisation of the single SiPM will be presented and compared with the old technology (NUV-SiPM) and with other SiPMs commercially available. The NUV-HD SiPM will be tested in the pSCT (SchwarzschildCouder Telescope prototype) for CTA which is leading to a camera concept based on 8 x 8 NUV-HD SiPM module as detection unit. An update on recent tests on the detectors arranged in this matrix configuration and on the front-end electronics will be given.n
Název v anglickém jazyce
Development of a SiPM based camera for Cherenkov Telescope Array
Popis výsledku anglicky
The Italian Institute of Nuclear Physics (INFN) is involved in the development of a prototype for a SiPM-based camera for the Cherenkov Telescope Array (CTA), a new generation of telescopes for ground - based gamma ray astronomy. In this framework, an R&D program for the development of SiPMs suitable for Cherenkov light detection (Near-Ultraviolet SiPMs) has been carried out. The developed device is a High Density NUV-SiPM based on a micro cell of 30 mu m x 30 mu m and 6 mm x 6 mm area produced by Fondazione Bruno Kessler (FBK). A full characterisation of the single SiPM will be presented and compared with the old technology (NUV-SiPM) and with other SiPMs commercially available. The NUV-HD SiPM will be tested in the pSCT (SchwarzschildCouder Telescope prototype) for CTA which is leading to a camera concept based on 8 x 8 NUV-HD SiPM module as detection unit. An update on recent tests on the detectors arranged in this matrix configuration and on the front-end electronics will be given.n
Klasifikace
Druh
D - Stať ve sborníku
CEP obor
—
OECD FORD obor
10303 - Particles and field physics
Návaznosti výsledku
Projekt
—
Návaznosti
—
Ostatní
Rok uplatnění
2017
Kód důvěrnosti údajů
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Údaje specifické pro druh výsledku
Název statě ve sborníku
Nuclear and Particle Physics Proceedings
ISBN
—
ISSN
2405-6014
e-ISSN
—
Počet stran výsledku
4
Strana od-do
55-58
Název nakladatele
Elsevier Science BV
Místo vydání
Amsterdam
Místo konání akce
Ischia
Datum konání akce
4. 7. 2016
Typ akce podle státní příslušnosti
WRD - Celosvětová akce
Kód UT WoS článku
000442844400012