Journal Article/Report/Contribution to a conference proceedings PUBDB-2015-00598

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Highlights from the Pierre Auger Observatory

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2014
Springer New York New York, NY

33rd International Cosmic Ray Conference, ICRC2013, Rio de JaneiroRio de Janeiro, Brazil, 2 Jul 2013 - 9 Jul 20132013-07-022013-07-09 Brazilian journal of physics 44(5), 560 - 570 () [10.1007/s13538-014-0218-6]
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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.

Classification:

Contributing Institute(s):
  1. Cherenkov Telescope Array (ZEU-CTA)
Research Program(s):
  1. 523 - High-energy gamma ray astronomy (POF2-523) (POF2-523)
Experiment(s):
  1. No specific instrument

Appears in the scientific report 2014
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Highlights from the Pierre Auger Observatory
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