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@INPROCEEDINGS{LetessierSelvon:206065,
author = {Letessier-Selvon, Antoine},
collaboration = {Pierre {Auger Collaboration}},
title = {{H}ighlights from the {P}ierre {A}uger {O}bservatory},
journal = {Brazilian journal of physics},
volume = {44},
number = {5},
issn = {1678-4448},
address = {New York, NY},
publisher = {Springer New York},
reportid = {PUBDB-2015-00598, arXiv:1310.4620},
pages = {560 - 570},
year = {2014},
abstract = {The Pierre Auger Observatory is the world's largest cosmic
ray observatory. Our current exposure reaches nearly 40,000
km$^2$ str and provides us with an unprecedented quality
data set. The performance and stability of the detectors and
their enhancements are described. Data analyses have led to
a number of major breakthroughs. Among these we discuss the
energy spectrum and the searches for large-scale
anisotropies. We present analyses of our X$_{max}$ data and
show how it can be interpreted in terms of mass composition.
We also describe some new analyses that extract mass
sensitive parameters from the 100\% duty cycle SD data. A
coherent interpretation of all these recent results opens
new directions. The consequences regarding the cosmic ray
composition and the properties of UHECR sources are briefly
discussed.},
month = {Jul},
date = {2013-07-02},
organization = {33rd International Cosmic Ray
Conference, Rio de Janeiro (Brazil), 2
Jul 2013 - 9 Jul 2013},
cin = {ZEU-CTA},
ddc = {530},
cid = {I:(DE-H253)ZEU-CTA-20120731},
pnm = {523 - High-energy gamma ray astronomy (POF2-523)},
pid = {G:(DE-HGF)POF2-523},
experiment = {EXP:(DE-MLZ)NOSPEC-20140101},
typ = {PUB:(DE-HGF)16 / PUB:(DE-HGF)29 / PUB:(DE-HGF)8},
eprint = {1310.4620},
howpublished = {arXiv:1310.4620},
archivePrefix = {arXiv},
SLACcitation = {$\%\%CITATION$ = $arXiv:1310.4620;\%\%$},
UT = {WOS:000342165000015},
doi = {10.1007/s13538-014-0218-6},
url = {https://bib-pubdb1.desy.de/record/206065},
}