Material for the analyses presented in "Arrival Directions of Cosmic Rays above 32 EeV from Phase One of the Pierre Auger Observatory"

Material for the analyses presented in "Arrival Directions of Cosmic Rays above 32 EeV from Phase One of the Pierre Auger Observatory "

This material includes the codes used to produce the results reported in the paper. A detailed description of the code can be found in appendix B of the paper and in the README file in the code. This material also includes the catalogs used for targeted searches of correlations. These are described in detail in the appendix C of the paper.

Required externals

This code is mostly written in C++ and requires some external software to work:

- Cern ROOT v6.xx {https://root.cern} is needed in all of the analyses to create and fill histograms, functions, and use formulas.

- HEALPix v3.xx {https://healpix.sourceforge.io/downloads.php} is a sky pixelization software needed in the blind and catalog-based searches.

- Python3 or Python 2.7 is necessary for recursion scripts and figure plotting.

Disclaimer

• This material is released under the (CC BY-SA 4.0) International License.

• This material has a unique DOI that you are requested to cite in any applications or publications.

• The Auger Collaboration does not endorse any work, scientific or otherwise, produced using this material, even if available on, or linked from, this portal.

• If you are interested in joining or working with the Auger Collaboration, please contact auger-join-request@auger.unam.mx.

Policy 

The policy of the Auger Collaboration on Data Release and Open Access can be found here.

Contact

For any question/doubt about this material, feel free to write to spokespersons@auger.org