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@INPROCEEDINGS{Travnicek:296683,
author = {Travnicek, Petr},
collaboration = {Pierre {Auger Collaboration}},
title = {{R}esults of the {P}ierre {A}uger {O}bservatory: {A}spects
related to hadronic interaction models},
address = {Hamburg},
publisher = {DESY},
reportid = {PUBDB-2016-01574, arXiv:0902.0377. DESY-PROC-2009-01},
pages = {211-216},
year = {2009},
abstract = {The southern part of the Pierre Auger Observatory in
Argentina is now fully completed and already provides world
unique data samples ofthe cosmic ray showers in the energy
range from 10$^{18}$eV till above 10$^{20}$eV. In order to
avoid a strong dependency on MC simulations forenergy
calibration, the experiment combines two techniques: surface
detector arrays and fluorescence telescopes. However, the i
nterpretation of some measured quantities such as mean
shower maximum in terms of chemical composition of cosmic
rays, naturally dependson MC simulations and models of
hadronic interactions at extremely high energies. This
contribution describes selected results of the Pierre Auger
Observatory and pinpoints several issues where the models of
hadronic interactions play a very important role or can be
even tested at energies far from the reach of current
accelerators.},
month = {Sep},
date = {2008-09-15},
organization = {38th International Symposium on
Multiparticle Dynamics, Hamburg
(Germany), 15 Sep 2008 - 20 Sep 2008},
cin = {CMS},
ddc = {530.143},
cid = {I:(DE-H253)CMS-20120731},
pnm = {Experiments at LHC (other) (POF1-510)},
pid = {G:(DE-H253)POF1-LHC-Exp.-(other)-20130405},
experiment = {EXP:(DE-H253)LHC-Exp-other-20150101},
typ = {PUB:(DE-HGF)29 / PUB:(DE-HGF)8},
eprint = {0902.0377},
howpublished = {arXiv:0902.0377},
archivePrefix = {arXiv},
SLACcitation = {$\%\%CITATION$ = $arXiv:0902.0377;\%\%$},
UT = {WOS:00},
doi = {10.3204/DESY-PROC-2009-01/73},
url = {https://bib-pubdb1.desy.de/record/296683},
}