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This code allows visualizing calculated energy fluences using Christian Glaser's geoceLDF package for various types of arrays. A custom array can be also used. Use files in CSV format where the first column is the station number and the following three are the stations x,y, and z coordinates.

Prerequisites:

Do not forget to add them to your python environmental variable $PYTHONPATH! E.g.:

export PYTHONPATH=$PYTHONPATH"/home/tomas/github/work:/home/tomas/github/work/geoceLDF:/home/tomas/github/work/radiotools:"
  • other prerequisites can be installed standardly via python -m pip install other_prerequisity

The average Xmax values in file "Xmax.dat" used in the calculation of the energy fluence were taken from ref.[1] up to lg(ECR) = 19.55 and from ref.[2] up to lg(ECR) = 19.85 and, for the highest energies extrapolated from [2]. Values were directly taken from Pierre Auger Collaboration's Internal publication GAP 2020-008 authored by A. Saftoiu and T. Huege.
[1] A. AAb et al. Pierre Auger Collaboration, Phys. Rev. D 90 (2014) 122005; arXiv:1409.4809v3.
[2] P. Sanchez-Lucas et al. Pierre Auger Collaboration, ICRC2017 Busan, Korea; arXiv:1708.06592v2.

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Tool for displaying analytically calculated quantities at detector arrays

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