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

Kód výsledku v 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>

Výsledek na webu

<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>

Jazyk výsledku

angličtina

Název v původním jazyce

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

Popis výsledku v původním jazyce

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

Název v anglickém jazyce

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

Popis výsledku anglicky

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

Druh

D - Stať ve sborníku

CEP obor

—

OECD FORD obor

10303 - Particles and field physics

Projekt

—

Návaznosti

—

Rok uplatnění

2018

Kód důvěrnosti údajů

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

Název statě ve sborníku

Proceedings of SPIE

ISBN

9781510619678

ISSN

0277-786X

e-ISSN

1996-756X

Počet stran výsledku

20

Strana od-do

1-20

Název nakladatele

SPIE

Místo vydání

Bellingham

Místo konání akce

Austin, Texas

Datum konání akce

10. 6. 2018

Typ akce podle státní příslušnosti

WRD - Celosvětová akce

Kód UT WoS článku

000452669100020