Depth of Maximum of Air-Shower Profiles at the Pierre Auger Observatory: Measurements at Energies above 10^17.8 eV
arXiv:1409.4809 · doi:10.1103/PhysRevD.90.122005
Abstract
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 telescopes of the Pierre Auger Observatory. The analysis method for selecting a data sample with minimal sampling bias is described in detail as well as the experimental cross-checks and systematic uncertainties. Furthermore, we discuss the detector acceptance and the resolution of the Xmax measurement and provide parameterizations thereof as a function of energy. The energy dependence of the mean and standard deviation of the Xmax-distributions are compared to air-shower simulations for different nuclear primaries and interpreted in terms of the mean and variance of the logarithmic mass distribution at the top of the atmosphere.
published version PRD
References in corpus (11)
- One-dimensional Hybrid Approach to Extensive Air Shower Simulation
- Measurement of the proton-air cross-section at TeV with the Pierre Auger Observatory
- The Cosmic Ray Energy Spectrum Observed with the Surface Detector of the Telescope Array Experiment
- The Offline Software Framework of the Pierre Auger Observatory
- New facts about muon production in Extended Air Shower simulations
- Hadronic Multiparticle Production at Ultra-High Energies and Extensive Air Showers
- A dip in the UHECR spectrum and the transition from galactic to extragalactic cosmic rays
- Reconstruction of Longitudinal Profiles of Ultra-High Energy Cosmic Ray Showers from Fluorescence and Cherenkov Light Measurements
- On the measurement of the proton-air cross section using air shower data
- Systematic uncertainties in air shower measurements from high-energy hadronic interaction models
- Atmospheric multiple scattering of fluorescence and Cherenkov light emitted by extensive air showers
Cited by in corpus (6)
- Escape model for Galactic cosmic rays and an early extragalactic transition
- Neutron β-decay as the origin of IceCube's PeV (anti)neutrinos
- Simulations of reflected radio signals from cosmic ray induced air showers
- Cosmic ray propagation with CRPropa 3
- Study of Dispersion of Mass Distribution of Ultra-High Energy Cosmic Rays using a Surface Array of Muon and Electromagnetic Detectors
- Alternative description of particle shower longitudinal profile