We present the first public code for semi-analytical calculation of the γ-ray flux astrophysical J-factor from dark matter annihilation/decay in the Galaxy, including dark matter substructures. The core of the code is the calculation of the line of sight integral of the dark matter density squared (for annihilations) or density (for decaying dark matter). The code can be used in three modes: i) to draw skymaps from the Galactic smooth component and/or the substructure contributions, ii) to ca...
Title of program: CLUMPY
Catalogue Id: AEKS_v1_0
Nature of problem
Calculation of γ-ray signal from dark matter annihilation (resp. decay). This involves a particle physics term and an astrophysical one. The focus here is on the latter.
Versions of this program held in the CPC repository in Mendeley Data
AEKS_v1_0; CLUMPY; 10.1016/j.cpc.2011.10.017
AEKS_v2_0; CLUMPY; 10.1016/j.cpc.2015.11.012
This program has been imported from the CPC Program Library held at Queen's University Belfast (1969-2018)
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