Aldée Charbonnier¹, Céline Combet^2,3, David Maurin³

¹(LPNHE/IN2P3/CNRS/Universités Paris VI et VII) ²(Dept. of Physics and Astronomy, University of Leicester, UK)
³(LPSC/CNRS/IN2P3, Université Joseph Fourier Grenoble 1, INPG)

aldee@lpnhe.in2p3.fr
celine.combet@lpsc.in2p3.fr
dmaurin@lpsc.in2p3.fr

If you use CLUMPY, please cite:
Charbonnier, Combet & Maurin, Comp. Phys. Comm. 183, 656 (2012)________________________________________

09/2011 - First release (Version 2011.09)
Hi guys!

We hope you will enjoy using CLUMPY whether you are

an experimentalist looking for realistic $\gamma$ -ray skymaps to calculate your new instrument sensitivity, or simply to use them in model/template analyses;
an astrophysicist, e.g. working on the DM content of dSphs, who wishes to calculate the J factor;
a theoretician who wants to plug his/her preferred particle physics model and see what is the corresponding $\gamma$ -ray flux in the Galaxy/dSph, etc.

To install the code and to have a quick overview before getting started, please visit the following pages:

Introduction - J-factor calculation and conventions
Downloads - tar.gz archive of the code
README - Follow the instructions to install CLUMPY
Examples - Examples and plots to quickly check CLUMPY once installed

If you believe that you have a module that would be a bonus for a future CLUMPY release, feel free to contact us to discuss the matter (and thus possibly join the crew).

The CLUMPY crew
Aldée, Céline, and David