On
“Anisotropy studies
around the
Abstract:
Data from the
Pierre Auger Observatory have been analyzed to search for anisotropies near the
direction of the galactic center in the energy range
from 0.8 to 3.2 EeV. In this region of the sky the
statistics accumulated by the Observatory are already larger than that of any
previous experiment. Using both the data sets from the surface detector and the
hybrid data sets (events detected simultaneously by the surface detector and
the fluouorescence detector) we do not find any
significant excess. Our results do not support previous findings of localized
excesses in the AGASA and SUGAR data. We set an upper bound on the flux of
cosmic rays arriving within a few degrees from the galactic center
for this energy range. We also have searched for correlations of cosmic ray
arrival directions with the galactic plane and the super-galactic plane at
energies in the range 1-5 EeV and above 5 EeV respectively. We have found no significant excess.
(“E. Majorana” room)