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@INPROCEEDINGS{Kunnas:315087,
author = {Kunnas, Maike Helena and Astapov, I. and Bezyazeekov, P.
and Bogdanov, A. and Boreyko, V. and Brückner, M. and
Budnev, N. and Chiavassa, A. and Chvalaev, O. and Gress, O.
and Gress, T. and Grishin, O. and Dyachok, A. and Epimakhov,
Sergey and Fedorov, O. and Gafarov, A. and Gorbunov, N. and
Grebenyuk, V. and Grinuk, A. and Horns, Dieter and Ivanova,
A. and Kalinin, A. and Karpov, N. and Kalmykov, N. and
Kazarina, Y. and Kirichkov, N. and Kiryuhin, S. and
Kokoulin, R. and Komponiest, K. and Konstantinov, A. and
Korosteleva, E. and Kozhin, V. and Kuzmichev, L. and Lenok,
V. and Lubsandorzhiev, B. and Lubsandorzhiev, N. and
Mirgazov, R. and Mirzoyan, R. and Monkhoev, R. and
Nachtigall, Rayk and Osipova, E. and Pakhorukov, A. and
Panasyuk, M. and Pankov, L. and Petrukhin, A. and Platonov,
V. and Poleschuk, V. and Popova, E. and Porelli, Andrea and
Postnikov, E. and Prosin, V. and Ptuskin, V. and Rubtsov, G.
and Pushnin, A. and Samoliga, V. and Satunin, P. and
Semeney, Yu. and Silaev, A. and Silaev, A. and Skurikhin, A.
and Slucka, V. and Spiering, Christian and Sveshnikova, L.
and Tabolenko, V. and Tarashansky, B. and Tkachenko, A. and
Tkachev, L. and Tluczykont, Martin and Voronin, D. and
Wischnewski, Ralf and Zagorodnikov, A. and Zurbanov, V. and
Yashin, I.},
title = {{S}imulation of imaging air shower {C}herenkov telescopes
as part of the {TAIGA} {P}roject},
address = {Hamburg},
publisher = {Verlag Deutsches Elektronen-Synchrotron},
reportid = {PUBDB-2016-05622},
isbn = {978-3-945931-08-0},
series = {DESY-PROC},
pages = {143-150},
year = {2016},
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.},
month = {Mar},
date = {2016-03-17},
organization = {Magellan Workshop, Hamburg (Germany),
17 Mar 2016 - 18 Mar 2016},
cin = {ZEU-EXP/AT},
cid = {$I:(DE-H253)ZEU-EXP_AT-20120731$},
pnm = {613 - Matter and Radiation from the Universe (POF3-613)},
pid = {G:(DE-HGF)POF3-613},
experiment = {EXP:(DE-MLZ)External-20140101},
typ = {PUB:(DE-HGF)8 / PUB:(DE-HGF)7},
UT = {WOS:00},
doi = {10.3204/DESY-PROC-2016-05/33},
url = {https://bib-pubdb1.desy.de/record/315087},
}