CLUMPY v3: $\gamma$-ray and $\nu$ signals from dark matter at all scales
Résumé
We present the third release of the CLUMPY code for calculating γ -ray and ν 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 γ -ray absorption up to high redshift. For more flexibility and consistency, dark matter halo masses and concentrations are now defined with respect to a user-defined overdensity Δ . We have also made changes for the user’s benefit: distribution and versioning of the code via git , less dependencies and a simplified installation, better handling of options in run command lines, consistent naming of parameters, and a new Sphinx documentation at http://lpsc.in2p3.fr/clumpy/ .