Depth of maximum of air-shower profiles at the Pierre Auger Observatory. II. Composition implications

A Aab, P Abreu, M Aglietta, EJ Ahn, I Al Samarai… - Physical Review D, 2014 - APS
Using the data taken at the Pierre Auger Observatory between December 2004 and
December 2012, we have examined the implications of the distributions of depths of …

Measurement of the cosmic Flux from 0.5 GeV to 1 TeV with the Alpha Magnetic Spectrometer (AMS-02) on the International Space Station

V Vagelli - 2014 - cds.cern.ch
The measurement of positrons and electrons (e+/-) in cosmic rays provides fundamental
information about the origin and the propagation of cosmic rays in the Galaxy. The interest in …

Different approaches to determine the composition of the ultra-high energy cosmic rays in the Pierre Auger Observatory

MB Otano - 2014 - theses.hal.science
The motivation of this PhD thesis is to improve the capabilities to determine the mass
composition of the ultra-high energy cosmic rays in the Pierre Auger Observatory. The …

Depth of maximum of air-shower profiles at the Pierre Auger Observatory

MT Dova, PM Hansen, CG Jarne, AG Mariazzi… - Physical Review …, 2014 - sedici.unlp.edu.ar
We report a study of the distributions of the depth of maximum, Xmax, of extensive air-
shower profiles with energies above 10 17.8 eV as observed with the fluorescence …

[PDF][PDF] Prospect towards Survey of Astronomical ντ Sources

GWS Hou, M Sasaki - UNIVERSE-TAIPEI, 2014 - s3.cern.ch
By separating ντ→ τ conversion from τ-shower generation, the Earth-skimming ντ method
allows for huge target mass and detection volume simultaneously. In part motivated by …

Depth of maximum of air-shower profiles at the Pierre Auger Observatory. I. Measurements at energies above 10¹⁷. ⁸ eV

A Aab, P Abreu, M Aglietta, E Ahn, I Al Samarai… - 2014 - hekyll.services.adelaide.edu.au
We report a study of the distributions of the depth of maximum, Xmax, of extensive air-
shower profiles with energies above 1017.8 eV as observed with the fluorescence …