Observations of Ultra-High Energy Cosmic Rays
arXiv:astro-ph/0511800 · doi:10.1088/1742-6596/39/1/100
Abstract
The status of measurements of the arrival directions, mass composition and energy spectrum of cosmic rays above 3 x 10^18 eV (3 EeV) is reviewed using reports presented at the 29th International Cosmic Ray Conference held in Pune, India, in August 2005. The paper is based on a plenary talk given at the TAUP2005 meeting in Zaragoza, 10 - 14 September 2005.
7 pages and two figures
References in corpus (4)
- Study of Small-Scale Anisotropy of Ultrahigh Energy Cosmic Rays Observed in Stereo by HiRes
- Upper limit on the photon fraction in highest-energy cosmic rays from AGASA data
- Search for Point Sources of Ultra-High Energy Cosmic Rays Above 40 EeV Using a Maximum Likelihood Ratio Test
- The mass composition of cosmic rays above 10^17 eV