Home > Publications database > Simulation of imaging air shower Cherenkov telescopes as part of the TAIGA Project |
Contribution to a conference proceedings/Contribution to a book | PUBDB-2016-05622 |
; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ;
2016
Verlag Deutsches Elektronen-Synchrotron
Hamburg
ISBN: 978-3-945931-08-0
This record in other databases:
Please use a persistent id in citations: doi:10.3204/DESY-PROC-2016-05/33 doi:10.3204/DESY-PROC-2016-05/33
Abstract: The Tunka Advanced International Gamma-ray and Cosmic ray Astrophysics (TAIGA) project aims at observation of cosmic rays beyond 100 TeV and gamma rays above 1 TeV via observation of the extensive air showers (EAS) caused in the atmosphere. Two common detection techniques are timing arrays and imaging air shower cherenkov telescopes (IACT). Timing arrays yield good directional and energy reconstruction, but provide only mediocre gamma-hadron-separation at their energy threshold. IACTs are good at separation, but since a stereoscopic view of a shower is needed for high reconstruction accuracy, it is difficult to achieve the large effective areas needed for ultra high energy observations. In this work we present the simulations performed to explore and optimize our IACT design and the first steps towards hybrid reconstruction.
![]() |
The record appears in these collections: |
Book/Proceedings/Report
Proceedings, Magellan Workshop : Connecting Neutrino Physics and Astronomy : Hamburg, Germany, March 17-18, 2016
Magellan Workshop, HamburgHamburg, Germany, 17 Mar 2016 - 18 Mar 2016
Hamburg : Verlag Deutsches Elektronen-Synchrotron, DESY-PROC 1-228 (2016) [10.3204/DESY-PROC-2016-05]
Files
Fulltext
BibTeX |
EndNote:
XML,
Text |
RIS