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Some doubts have been expressed about low energy supersymmetry (SUSY)following the first run of the LHC. In this talk I will try to present a moreupbeat view based on data, rather than theoretical expectations. In particular,I will make the following points: (a) in my opinion the most attractivecandidate for dark matter (DM) is now the lightest neutralino with mass around1 TeV and with well defined properties (a nearly pure higgsino). This followsprimarily from a combination of the properties of the discovered Higgs boson,in particular its mass close to 125 Gev, and the relic density of dark matter,and is most clearly visible in the context of unified, or constrained, SUSYframeworks, although the DM candidate is quite generic; (b) this DM candidatewill be nearly fully tested in forthcoming one-tonne DM underground searchdetectors; (c) the CMSSM will be nearly fully tested in the next few years by acombination of expected data from LHC experiments and from direct DM searches,as well as potentially also by the Cherenkov Telescope Array; (d) ifnaturalness plays any real role in SUSY (which remains unclear), then theamount of fine tuning, which is very large in simple models like the CMSSM, canbe significantly reduced (even down to 1 in 20) with properly selected boundaryconditions at the unification scale; (e) the (g-2) muon anomaly can beaccommodated not only in the context of the general MSSM but also of someunified SUSY models with some superpartners to be within reach of the LHC.

Looking for supersymmetry: ~1 Tev WIMP and the power of complementarity in LHC and dark matter searches