We present a feasibility study of ρT and aT production using the ρT/aT→WZ→lllν final state. Such a signature is found in low scale walking Technicolor models. We perform this study using CMS fast simulation samples and conclude that it is possible to observe ρT with masses up to 500~GeV in data samples ranging from 2-10~fb−1 of integrated luminosity. We also find that the aT→WZ process may be seen under the assumptions that MaT≃1.1MρT (for MρT=500 GeV) and that the MET resolution from data will be in reasonable agreement with the simulation