TY  - CHAP
AU  - Maier, Gernot
TI  - Appendix: Simulating CTA
CY  - Singapore
PB  -  World Scientific 
M1  - PUBDB-2019-04626
SN  - 978-981-327-008-4
T2  - 1712968
SP  - 299 - 300
PY  - 2019
N1  - Includes bibliographical references
AB  - The expectations for the scientific capabilities of CTA presented in this document are based on sensitivity and response functions derived from detailed Monte Carlo simulations of the CTA observatory. The simulations model extensive air showers initiated by high-energy (HE) primary particles (gamma rays or background cosmic-ray nuclei and electrons), the Cherenkov light production by the shower particles, and the measurement processes of imaging atmospheric Cherenkov telescopes…
KW  - Cherenkov counter: atmosphere (INSPIRE)
KW  - nucleus: cosmic radiation (INSPIRE)
KW  - showers: atmosphere (INSPIRE)
KW  - numerical calculations: Monte Carlo (INSPIRE)
KW  - radiation: Cherenkov (INSPIRE)
KW  - Cherenkov Telescope Array (INSPIRE)
KW  - observatory (INSPIRE)
KW  - sensitivity (INSPIRE)
KW  - background (INSPIRE)
KW  - gamma ray (INSPIRE)
KW  - electron (INSPIRE)
KW  - imaging (INSPIRE)
KW  - air (INSPIRE)
LB  - PUB:(DE-HGF)7
DO  - DOI:10.1142/9789813270091_0015
UR  - https://bib-pubdb1.desy.de/record/428603
ER  -