Speaker
Dr
Viviana Scherini
(University of Milano and INFN Milano (Italy))
Description
The Pierre Auger Observatory has a significant sensitivity to search for ultra-high energy photons using data from the ground detector alone or in hybrid mode. Recent upper limits on the photon flux are already below the percent-level with regard to the total flux. The current status and details of the analysis methods are presented.
Primary author
Dr
Viviana Scherini
(University of Milano and INFN Milano (Italy))
Co-author
P. Auger Collaboration
(Malargue, Argentina)
