http://arxiv.org/abs/1806.08639
We present the third release of the CLUMPY code for calculating $\gamma$-ray and neutrino signals from annihilations or decays in dark matter structures. This version includes the mean extragalactic signal with several pre-defined options and keywords related to cosmological parameters, mass functions for the dark matter structures, and $\gamma$-ray absorption up to high redshift. For more flexibility and consistency, dark matter masses and concentration are now defined with respect to a user-defined overdensity $\Delta$. We have also made changes for the user’s benefit: it includes a better handling of options in run command lines, consistent naming of parameters, distribution of the code via git, and an updated documentation at this http URL
M. Hütten, C. Combet and D. Maurin
Mon, 25 Jun 18
6/54
Comments: 10 pages, 5 figures. Submitted to Computer Physics Communications. Code and documentation available from this http URL
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