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000206065 0881_ $$aarXiv:1310.4620
000206065 088__ $$2arXiv$$aarXiv:1310.4620
000206065 1001_ $$0P:(DE-HGF)0$$aLetessier-Selvon, Antoine$$b0$$eCorresponding Author
000206065 1112_ $$a33rd International Cosmic Ray Conference$$cRio de Janeiro$$d2013-07-02 - 2013-07-09$$gICRC2013$$wBrazil
000206065 245__ $$aHighlights from the Pierre Auger Observatory
000206065 260__ $$aNew York, NY$$bSpringer New York$$c2014
000206065 300__ $$a560-570
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000206065 520__ $$aThe 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.
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000206065 7001_ $$0P:(DE-HGF)0$$aPierre Auger Collaboration$$b1$$eCollaboration author
000206065 773__ $$0PERI:(DE-600)1493260-x$$a10.1007/s13538-014-0218-6$$gVol. 44, no. 5, p. 560 - 570$$n5$$p560 - 570$$tBrazilian journal of physics$$v44$$x1678-4448$$y2014
000206065 7870_ $$0PUBDB-2015-00596$$aLetessier-Selvon, Antoine et.al.$$d2013$$iIsParent$$rICRC2013;  arXiv:1310.4620$$tHighlights from the Pierre Auger Observatory
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