Speaker
Mrs
Isabelle Lhenry-Yvon
(IPN Orsay, CNRS IN2P3)
Description
The Pierre Auger Observatory, located in Argentina, has been detecting ultra-high energy cosmic rays for more than ten years. The combination of a large surface detector array and fluorescence telescopes provides a substantial improvement in energy calibration and extensive air shower measurements, resulting in data of unprecedented quality in the energy range from 0.1 EeV up to 100 EeV. A review of main results from the Pierre Auger Observatory is presented with a particular focus on the energy spectrum measurements , mass composition studies and the arrival directions analyses.
| Experimental Collaboration | Pierre Auger Collaboration |
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Primary author
Mrs
Isabelle Lhenry-Yvon
(IPN Orsay, CNRS IN2P3)
