Techniques to study cosmic ray anisotropies
arXiv:0902.3601
Abstract
These lectures review some of the techniques used to analyze the arrival direction distribution of Cosmic Rays, and some relevant results on the field.
To appear in the Proceedings of the Third School on Cosmic Rays and Astrophysics, Arequipa, Peru
References in corpus (13)
- Correlation of the highest energy cosmic rays with nearby extragalactic objects
- Observation of the suppression of the flux of cosmic rays above 4x10^19eV
- Correlation of the highest-energy cosmic rays with the positions of nearby active galactic nuclei
- Anisotropy and Corotation of Galactic Cosmic Rays
- Observation of the Anisotropy of 10 TeV Primary Cosmic Ray Nuclei Flux with the Super-Kamiokande-I Detector
- Cosmic Ray Anisotropy Analysis with a Full-Sky Observatory
- The toes of the ultra high energy cosmic ray spectrum
- Anisotropy studies around the galactic centre at EeV energies with the Auger Observatory
- On the ultra-high energy cosmic ray horizon
- Observation by an Air-Shower Array in Tibet of the Multi-TeV Cosmic-Ray Anisotropy due to Terrestrial Orbital Motion Around the Sun
- Search for correlation of UHECRs and BL Lacs in Pierre Auger Observatory data
- Search for large-scale anisotropies with the Auger Observatory
- Search for clustering of ultra high energy cosmic rays from the Pierre Auger Observatory