Maps are projected dark matter density and density squared, repectively, weighted by 4π the distance squared, as explained in the paper.

You can use these maps with your preferred particle physics model and analyse the result.

If you want to use our maps in your work, please cite our paper A.J.Cuesta et al. 2010 as well as the CLUES project from where we took the BOX160CR constrained realization of the Local Universe to produce the maps.

"Dark Matter Decay and Annihilation: CLUES from Fermi"

A.J.Cuesta, T.E.Jeltema, F.Zandanel, S.Profumo, F.Prada, G.Yepes, A.Klypin, Y.Hoffman, S.Gottlober, J.Primack, M.A.Sanchez-Conde & C.Pfrommer

APJ Letters 726, L6, 2011

There is an ERRATUM, see APJ, ADS or the Appendix of the PDF and ARXIV versions. The maps available here are correct since July 26th 2011.

[PDF] [ARXIV] [ADS]

For any question please contact: antonio.cuesta@yale.edu (A.J.Cuesta), tesla@ucolick.org (T.E.Jeltema) or fabio.zandanel@gmail.com (F.Zandanel)