These samples were obtained by the KISMET method (Killer Inference in Susy METeorology). For access to samples of the phenomenological (pMSSM) data used in arXiv:0906.0957, please email Shehu AbdusSalam shehu@ictp.it.
Alternatively, for CMSSM samples, use: arXiv:0705.0487. If you use them, please cite that paper. You might also like to look at the preceeding papers on the same topic: [1 | 2 | 3]. The SLHA files come from independent samplings of the MCMC samples that they are listed with.
[ Tarred gzipped files | root file | SLHA format files ]:
The density of points in parameter space is proportional to the posterior probability of the point. The fits are described in the paper, and have had the dark matter, (g-2)_mu, B_s->mu mu, MW, sin^2 theta_l, mt, mb, alphas, BR(b->s gamma) and sparticle/Higgs direct search limits applied to them. Each point in the sample is a line of the file, organised into a list of numbers, in the following order: