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. 2014 Dec 17;74(12):3212. doi: 10.1140/epjc/s10052-014-3212-9

Table 2.

The best-fit points found in global fits in the CMSSM, the NUHM1 and the NUHM2, using the same experimental constraints (and their theoretical interpretations): the difference in the CMSSM best-fit from that found in [19] is due to using the updated ATLAS jets + /ET constraint [10]. We note that the overall likelihood functions in all the models are quite flat, so that the precise locations of the best-fit points are not very significant, and for this reason we do not quote uncertainties. The p-values quoted would have the interpretations of probabilities if the likelihood functions given by the χ2 statistics were Gaussian

Model χ2/dof p-value (%) m0 (GeV) m1/2 (GeV) A0 (GeV) tanβ mHu2 (GeV2) mHd2 (GeV2)
CMSSM 35.0/23 5.2 420 970 3000 14 =m02 =m02
NUHM1 32.7/22 6.6 1380 3420 -3140 39 1.33×107 =mHu2
NUHM2 32.5/21 5.2 -490 1730 4930 21 -5.28×107 -4.03×107