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The NO$\nu$A collaboration has constructed a 14,000 ton, fine-grained, low-Z,total absorption tracking calorimeter at an off-axis angle to an upgraded NuMIneutrino beam. This detector, with its excellent granularity and energyresolution and relatively low-energy neutrino thresholds, was designed toobserve electron neutrino appearance in a muon neutrino beam, but it also hasunique capabilities suitable for more exotic efforts. In fact, if an efficientupward-going muon trigger with sufficient cosmic ray background rejection canbe demonstrated, NO$\nu$A will be capable of a competitive indirect dark mattersearch for low-mass WIMPs. The cosmic ray muon rate at the NO$\nu$A fardetector is about 100 kHz and provides the primary challenge for triggering andoptimizing such a search analysis. The status of the NO$\nu$A upward-going muontrigger is presented.

Implementation of an upward-going muon trigger for indirect dark matter searches at the NO$\nu$A far detector