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We present the first public code for semi-analytical calculation of thegamma-ray flux astrophysical J-factor from dark matter annihilation/decay inthe Galaxy, including dark matter substructures. The core of the code is thecalculation of the line of sight integral of the dark matter density squared(for annihilations) or density (for decaying dark matter). The code can be usedin three modes: i) to draw skymaps from the Galactic smooth component and/orthe substructure contributions, ii) to calculate the flux from a specific halo(that is not the Galactic halo, e.g. dwarf spheroidal galaxies) or iii) toperform simple statistical operations from a list of allowed DM profiles for agiven object. Extragalactic contributions and other tracers of DM annihilation(e.g. positrons, antiprotons) will be included in a second release.

CLUMPY: a code for gamma-ray signals from dark matter structures