Performance optimization of the air shower simulation program for the Cherenkov Telescope Array

Result code in IS VaVaI

<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68378271%3A_____%2F19%3A00552422" target="_blank" >RIV/68378271:_____/19:00552422 - isvavai.cz</a>

Result on the web

<a href="https://www.epj-conferences.org/articles/epjconf/pdf/2019/19/epjconf_chep2018_05041.pdf" target="_blank" >https://www.epj-conferences.org/articles/epjconf/pdf/2019/19/epjconf_chep2018_05041.pdf</a>

DOI - Digital Object Identifier

<a href="http://dx.doi.org/10.1051/epjconf/201921405041" target="_blank" >10.1051/epjconf/201921405041</a>

Result language

angličtina

Original language name

Performance optimization of the air shower simulation program for the Cherenkov Telescope Array

Original language description

The Cherenkov Telescope Array (CTA), currently under construction, is the next-generation instrument in the field of very high energy gamma-ray astronomy. The first data are expected by the end of 2018, while the scientific operations will start in 2022 for a duration of about 30 years. In order to characterize the instrument response to the Cherenkov light emitted when cosmic ray showers develop in the atmosphere, detailed Monte Carlo simulations will be regularly performed in parallel to CTA operation.

Czech name

—

Czech description

—

Type

D - Article in proceedings

CEP classification

—

OECD FORD branch

10303 - Particles and field physics

Project

—

Continuities

—

Publication year

2019

Confidentiality

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

Article name in the collection

EPJ Web of Conferences

ISBN

—

ISSN

2100-014X

e-ISSN

—

Number of pages

9

Pages from-to

1-9

Publisher name

EDP Sciences

Place of publication

les Ulis

Event location

Sofia

Event date

Jul 9, 2018

Type of event by nationality

WRD - Celosvětová akce

UT code for WoS article

000570241300259