Auger group publications (January 2015-June 2017) [1] A. Aab et al. (Pierre Auger Collaboration). “A targeted search for point sources of EeV photons with the Pierre Auger Observatory”. Astrophys. J.

Aerosol monitoring is performed using two central laser- s (CLF/XLF), four elastic scattering lidar stations, two aerosol phase function monitors (APF) and two optical

To compute the Pierre Auger Observatory sensitivity to skimming neutrinos, an incident flux of ντ is injected in the earth at energies ranging from 10 17.. to

Atmospheric aerosols at the Pierre Auger Observatory : characterization and effect on the energy estimation for ultra-high energy cosmic rays... 1.2 Extensive

VEM-peak and C is a scale factor obtained from Monte Carlo simulation of the shower development [56]. In the present section, an effort is made to quantify the

The Observatory will consist when completed of 1600 water ˇ Cerenkov tanks and 24 fluorescence telescopes, organized in 4 sites, sampling ground particles and measuring fluores-

After presenting the Southern Auger site and its current status, we will describe the recent Auger results on the anisotropy studies, and the first estimate of the UHECR spectrum..

Here we first present two technical tools of prime importance to study UHECR anisotropies, namely: the arrival direction reconstruction of Auger Surface Detector events, and the

L’archive ouverte pluridisciplinaire HAL, est destinée au dépôt et à la diffusion de documents scientifiques de niveau recherche, publiés ou non, émanant des