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Journal Article/Report/Contribution to a conference proceedings | PUBDB-2015-00598 |
;
2014
Springer New York
New York, NY
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Please use a persistent id in citations: doi:10.1007/s13538-014-0218-6
Report No.: arXiv:1310.4620
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.
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Highlights from the Pierre Auger Observatory
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