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

Pierre Auger Collaboration

Abstract:

<strong>Material for the analyses presented in "Arrival Directions of Cosmic Rays above 32 EeV from Phase One of the Pierre Auger Observatory "</strong> 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. <strong>Required externals</strong> 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. <strong>Disclaimer</strong> 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. ... mehr


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Originalveröffentlichung
DOI: 10.5281/zenodo.6759610
Zugehörige Institution(en) am KIT Institut für Astroteilchenphysik (IAP)
Publikationstyp Forschungsdaten
Publikationsjahr 2022
Identifikator KITopen-ID: 1000155858
HGF-Programm 51.13.03 (POF IV, LK 01) Kosmische Strahlung Auger
Lizenz Creative Commons Namensnennung 4.0 International
Schlagwörter UHECR, Anisotropy, Astrophysics, Cosmic Rays
Art der Forschungsdaten Software
KIT – Die Forschungsuniversität in der Helmholtz-Gemeinschaft
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